2. DESCRIPTION OF THE CATALOG (TABLE 1): COLUMN HEADINGS

STAR DESIGNATION. Star designation derived from right ascension (hhmm) and declination (±ddmm) of the star.

CGCS. This is the number from the first column (No.) of Table 1 from the 2nd edition (CGCCS). We have not introduced a new running number to avoid overcrowding of identifiers for an object. For new entries the running numbers begin with No. 6001 and are given in the sequence of R.A.(2000).

RA(2000), DEC(2000). These are the equatorial coordinates, referred to the equinox and equator 2000.

<<In case of multiple finding lists, the coordinates are averages from multiple sources, heavily weighted in favor of the most accurate, if any. Where Ste is included among the designations, the star has almost invariably been measured for position at the Warner and Swasey Obs. on one or even more objective-prism plates, with a resulting precision of 1-2 arcseconds. The astrometric reduction procedure used by Stephenson is explained in Publs. Warner and Swasey Obs. Vol. 2, No. 4, Sec. II. More than 2000 stars of Table 1 have post CCCS position determinations done at the Warner and Swasey Observatory.>>

The coordinates are given to 0.1 sec in RA and 1 arcsec in DEC, notwithstanding the precision of the position of the object. The estimated precision class of the coordinates is indicated by precision in the last column. For many stars of CGCCS the equatorial coordinates have been improved on the basis of new determinations, e.g., by Aaronson et al. (1989, 1990), MacConnell (2000), Maehara & Soyano (1988, 1990), Soyano & Maehara (1991, 1993, 1999).

For more than 300 carbon stars equatorial coordinates were taken from the Hipparcos Catalogue after approximation to the format of this catalog. These stars can be recognized as bright stars with the highest precision class 0 in the last column of the Table.

b, v, i. << These are, as available, blue, visual and infrared magnitudes. The infrared magnitudes are normally the sort defined by a Kodak N-type photographic plate exposed through a filter similar to the Schott RG8 or 695 filter. Such infrared magnitudes are close to the system of Kron & Smith (1951), and have now been published for several thousand carbon stars. For b, v and i alike, the magnitudes essentially all come from photographic plates; thousands of them are based only upon an average plate calibration used for an entire survey. Thus the magnitudes are almost never accurate to 0.1 mag, to which they are commonly given, and errors of over a whole magnitude should be common, even discounting variability.>>

For some stars v magnitudes from Paupers et al. (1993) are used. For the newly added stars, especially for the infrared (or dusty) carbon stars, which are observed only in the infrared, column i gives red or near infrared magnitude in the shortest awailable wavelength with corresponding notation: R, J, H, K, L.

long, lat. <<This is galactic longitude and latitude, in the system currently in use.>> They are computed from RA(2000) and Dec(2000).

Spectrum. <<This column displays the earliest more reliable determinations of spectral type in the R/N notation. Here also are classifications in the scheme of Morgan & Keenan (1941); this scheme is still a good compact description of the spectrum. Sources of quoted classifications are coded here in parentheses; most of these are listed in the explanation of the “Designations” column, which is devoted to finding lists. Below we list abbreviations for papers consisting mainly of re-observation of stars selected from finding lists. We also include here the abbreviations HD and HDE which are occasionally cited under the “Spectrum” column.>> However, these abbreviations are omitted in the “Designations” column where a pure HD or HDE number is given.

These abbreviations are as follows.

Bidun	Bidelman, unpublished.
De	Dean (1976).
HD, HDE	Henry Draper Catalogue and the first extension, Harvard Annals 91-100. The second extension, HA 112, is cited as CannMay49.
Her52	Herbig (1952).
IRAS C	Little-Marenin et al. (1987)
K-M	Keenan & Morgan (1941)
Lund21	Lundmark (1921).
San41	Sanford (1941).
San	Sanford (1944).
Sh	Shane (1928).
War	Warner (1963).
WPB	Bidelman (1954).
Yam	Yamashita (1972, 1975).

Carbon star candidates in this column are marked by lower case c (Guglielmo et al. 1998 and references threin).

Designations. <<This gives the star's occurence in various finding lists, including unpublished ones. Some CCCS stars repeated here are still called unpublished, which means only that I had no reference to a separate publication when the CCCS went to press. For some of those stars, the CCCS is the only place they have been published; for others, they have since appeared in separate lists by their discoverers. In the latter case I have sometimes changed the discoverer designation to reflect separate subsequent publication, and sometimes not; in the great majority of cases, CCCS stars there called unpublished have since been confirmed in other surveys.

There are finding lists with no special concentration on carbon stars. These are the Bright Star Catalog number, cited, as in all editions of the Bright Star Catalog, as an HR number (and usually put at the head of the list); HD or HDE numbers (listed as a number without other characters); BD or CD numbers in a notation close to the usual one; and the GCVS designation. The intent was to give CD numbers only if the CD magnitude is 9.5 or brighter. Any CPD (Cape Photographic Durchmusterung) nos. in Table 1 are inadvertent unless spelled out as such, a fact due to the circumstance that carbon stars are red stars and the CD is red-biased, not only relative to the CPD but even, though this does not appear to be widely known, relative to the BD.

Other finding lists; an explanation for the coding of these follows. The largest unpublished ones are by Stephenson (Ste), a combination of stars now published in the CCCS and infrared survey products appearing in the present catalog; Sanduleak (Sndlk), whose entries are almost exclusively confined to CCCS stars; Victor Blanco (VB); and MacConnell (MacCon). Although there are several published MacConnell lists cited here, some of the “MacCons” may have since become separately published; but see also the special note under MacCon in the table to follow.

Coding: Whenever a number appears separated from the initial part of the designation by a blank space, the number is a published one assigned by the corresponding discoverer, hyphens if any separating table numbers from numbers within tables. Numbers following alphabetic abbreviations without a blank space represent the year of publication where this was for some reason helpful to me (generally, where the same author has produced more than one paper). So W58 1 means star No. 1 in a table of carbon stars in Westerlund (1958).>>

The abbreviations mean the following:

Aar89	Aaronson, Blanco, Cook, and Schechter (1989).
Aar90	Aaronson, Blanco, Cook, Olszewski, and Schechter (1990).
AbrGig89a	Abramyan and Gigoyan (1989a).
AbrGig89b	Abramyan and Gigoyan (1989b).
AbrGig90	Abramyan and Gigoyan (1990).
AbrGig93	Abramyan and Gigoyan (1993).
AbrGig94	Abramyan and Gigoyan (1994).
Ack	Ackermann (1970).
AFGL=CRL	Infrared sky survey, U.S. Air Force, Hanscom Field, MA.
AGHA97	Abramyan, Gigoyan, Hambaryan, and Azzopardi (1997).
AGSh95	Abramyan, Gigoyan, and Shakhbazyan (1995).
Akyol	Akyol et al. (1974).
Alb	Albers (1967).
Alks72	Alksne and Ozolina (1972).
All77	Allen, Hyland, Longmore, Caswell, Goss, and Haynes (1977).
ALR	Azzopardi et al. (1985).
ALRW91	Azzopardi, Lequeur, Rebeirot, and Westerlund (1991).
Balz56	Balz (1956).
Barb70	Barbier (1970).
BC -	Baldone Carbon star number, assigned at Baldone, Latvia:
BC 10 - BC 33	Alksne and Ozolina (1974),
BC 34 - BC 39	Daube and Ozolina (1974),
BC 40 - BC 49	Alksne and Ozolina (1975),
BC 50 - BC 62	Alksne and Ozolina (1976),
BC 63 - BC 77	Alksnis, Alksne, Ozolina, and Eglitis (1976),
BC 78 - BC 109	Alksnis, Alksne, and Ozolina (1977),
BC 110 - BC 184	Alksnis, Alksne, Ozolina, and Platais (1978),
BC 185	Platais (1979),
BC 186 - BC 200	Platais (1981),
BC 201 - BC 217	Alksne and Alksnis (1981),
BC 218 - BC 234	Alksne, Alksnis, and Eglitis (1981),
BC 235 - BC 245	Alksnis, Alksne, and Eglitis (1983),
BC 246 - BC 255	Alksnis and Ozolina (1983),
BC 256 - BC 272	Alksnis, Alksne, Platais, and Ozolina (1987),
BC 273 - BC 310	Alksnis, Alksne, Ozolina, and Platais (1988),
BC 311 - BC 318	Alksnis, Alksne, Ozolina, and Platais (1988),
BC 1 - BC 318	Alksne, Alksnis, Ozolina, and Platais (1989).
Bid80	Bidelman (1980).
BidMac	Bidelman and MacConnell (1973).
Blanc55	Blanco, Nassau et al. (1955).
B-M	Blanco and Munch (1955).
Bon75	Bond (1975).
Boes	Boeshaar, unpublished.
Bot91	Bothun, Elias, Macalpine, Matthews, Mould, Neugebauer, and Reid (1991).
BSD	The Bergedorfer Spektral-Durchmusterung (Schwassmann and Van Rhijn1935).
C	The Case infrared surveys at low galactic latitudes (Nassau and Blanco 1954, 1957; Blanco1958). The carbon star numbers are continuous from paper to paper.
Cann2	Cannon (1921).
Cann22	Cannon (1922).
Cann26	Cannon (1926).
CannMay38	Cannon and Mayall (1938).
CannMay49	Cannon and Mayall (1949). The Annie J. Cannon Memorial.
Catchp68	Catchpole (1968).
CCCS	Catalogue of Cool Carbon Stars, First ed. (Stephenson, 1973).
CCGCS	A General Catalogue of Cool Galactic Carbon Stars, Second ed.(Stephenson, 1989)
CH96	Cohen and Hitchon (1996).
CK77	Cohen and Kuhi (1977).
CohKuh	Cohen and Kuhi (1976).
Crg61	Cregg (1961).
Cut89	Cutri, Low, Kleinmann, Olszewski, Willner, Campbell, and Gillett (1989).
CWWVS	Cohen, Wainscoat, Walker, Volk, and Schwartz (1989).
CWWV96	Cohen, Wainscoat, Walker, and Volk (1996).
D	The Dearborn Observatory objective-prism surveys for red stars (Lee et al. 1940-44). The carbon stars thus found were abstracted as lists of exclusively carbon stars, in the papers just cited, and were duplicated in longer lists containing all red stars found; the D numbers given in Table 1 refer to the short lists, with one or two exceptions spelled out in the notes to the table. The notes also refer in other contexts to the “longer” Dearborn lists, with the meaning just explained. The "short" list numbers for carbon stars are continuous from paper to paper.
Daub71	Daube (1971).
DLKSH77	Dahn, Liebert, Kron, Spinrad, and Hintzen (1977).
Dol62	Dolidze (1962).
Dol68	Dolidze (1968).
Dol71a	Dolidze (1971a).
Dol71b	Dolidze (1971b).
Dril72	Drilling (1972).
Epc87	Epchtein, Le Bertre, Lepine, Margues dos Santos, Matsuura, and Picazzio (1987).
Epc90	Epchtein, Le Bertre, and Lepine (1990).
Esp	Espin (1924).
Fea97	Feast (1997).
Feast77	Feast et al. (1977).
Flem12	Fleming (1912).
Fou92	Fouque, Le Bertre, Epchtein, Guglielmo, and Kerchbaum (1992).
Fr75	Frogel, Dickinson, and Hyland (1975).
Fuen	Fuenmayor (1981).
FueSto95	Fuenmayor and Stock (1995).
GAA	Gigoyan, Hambaryan, and Azzopardi (1998).
GAM	Gigoyan, Azzopardi, and Muratorio (1999).
GBE98	Guglielmo, Le Betre, and Epchtein (1998).
GEAS97	Guglielmo, Epchtein, Arditti, and Sevre (1997).
GCVS	General Catalogue of Variable Stars Volumes I - III, 4 th ed. (1999).
GGHCG	Grasdalen, Gehrz, Hackwell, Castelaz, and Gullison (1983).
GH76	Gehrz and Hackwell (1976).
GigAmb	Gigoyan, Hambaryan (1996).
GJ93	Groenewegen and de Jong (1993).
GJB93	Groenewegen, de Jong, and Baas (1993).
GJBSW	Groenewegen, de Jong, van der Bliek, Slijkhuis, and Willems (1992).
GJG94	Groenewegen, de Jong, and Geballe (1994).
GMAC	Green, Margon, Anderson, and Cook (1994).
GMAM92	Green, Margon, Anderson, and MacConnell (1992).
GMM91	Green, Margon, and MacConnell (1991).
GOL97	Groenewegen, Oudmaijer, and Ludwig (1997).
Gor68	Gordon (1968).
GreMar90	Green and Margon (1990).
GreMar94	Green and Margon (1994).
Gug93	Guglielmo, Epchtein, Le Betre, Fouque, Hron, Kerschbaum, and Lepine (1993).
GWSK	Groenewegen, Whitelock, Smith, and Kerschbaum (1998).
Ha85	Hartwick and Cowley (1985).
HanBl	Hansen and Blanco (1975).
Har	Hardorp, Lubeck, and Stephenson (1972). Spectral type ER = early R, LN = Late N, etc.
Harw	Harwood (1962).
Hen	Rybski (1972). Most of the carbon stars discussed by Rybski were found on objective-prism plates by Henize, and by him assigned the numbers which Rybski refers to as Hen numbers and Stephensone quote in Table 1. There is no connection between these Hen numbers and others occurring in the literature--even in the case of the occasional Hen numbers for carbon stars cited by Wray (1966), who however, also assigns his own numbers and which are quoted in Table 1 as Wray.
IDS	Index Catalogue of Double Stars. Not mentioned if ADS number given.
JBGHJKL	Jones, Bryja, Gehrz, Harrison, Johnson, Klebe, and Lawrence (1990).
Jon78	Jones, Merrill, Puetter, and Willner (1978).
Joy98	Joyce (1998).
Krum	L. E. Krumenaker, unpublished. At Warner and Swasey we had by 1972 taken duplicate objective-prism plates of the northern Milky Way for about half of the fields surveyed by Hamburg in the Hamburg-Cleveland survey for luminous stars in the Northern Milky Way. Although carbon stars were identified and measured for position by the Hamburg workers, and eventually published (Hardorp et al. 1972), the Hamburg limiting magnitude for carbon stars was not very faint (cf. Hardorp et al. 1972). Hence Krumenaker searched for carbon stars on the new Case material already mentioned. On the other hand, the mag. limit for R/N classification is already fairly uniform between Hamburg and Cleveland (Stephenson 1989).
Krum75	Krumenacker (1975).
Kub	W. R. Kubinec, unpublished. These carbon stars are discussed by Kubinec, without position data, in Publs. Warner & Swasey Obs. 1, No. 3. He measured the approximate positions specially for Table 1.
Kur96	Kurtanidze, unpublished (1996).
KurNik88	Kurtanidze and Nikolashvili (1988).
KurNik88b	Kurtanidze and Nikolashvili (1988b).
KurNik89	Kurtanidze and Nikolashvili (1989).
KurNik90	Kurtanidze and Nikolashvili (1990).
KurNik2000	Kurtanidze and Nikolashvili (2000).
Kurt78	Kurtanidze (1978, 80, 80a, 81, 88).
Kurt80
Kurt80a
Kurt81
Kurt88
Kurtun	Kurtanidze, unpublished. Some of these may now be in prin
KurtWest	Kurtanidze and Westerlund (1980).
LE83	Lloyd Evans (1983).
LE90	Lloyd Evans (1990).
LE91	Lloyd Evans (1991).
LeB92	Le Bertre (1992).
LFOP93	Loup, Forveile, Omont, and Paul (1993).
Lit	Little-Marenin et al. (1987). These are carbon star classifications from IRAS spectra (11.2 micron SiC emission).
LKVR76	Low, Kurtz, Vrba, and Rieke (1976).
Lo74	Lockwood (1974).
LR77	Lebofsky and Rieke (1977).
LSKR78	Lebofsky, Sargent, Kleinmann, and Rieke (1978).
LSLSLCFB	Liebert, Schmidt, Lesser, Stepanian, Lipowetsky, Chaffee,Foltz, and Bergeron (1994).
MacCon	With running nos. 1-466, MacConnell (1988).
MacCon	MacConnell, unpublished, at least originally.
MacCon67	MacConnell (1967, 79, 81, 82).
MacCon79
MacCon81
MacCon82
MacCon97	MacConnell (1997).
MacCon2000	MacConnell, unpublished (2000).
MaeSoy	Maehara and Soyano (1986a).
MaeSoy2	Maehara and Soyano (1986b).
MaeSoy88	Maehara and Soyano (1988).
MaeSoy90	Maehara and Soyano (1990).
Marg	Margon et al. (1984).
May51	M. Walton Mayall (1951).
MayCann40	M. Walton Mayall and Cannon (1940).
Mayun	N. U. Mayall, unpublished, communicated to C.B.Stephenson by W. P.Bidelman.
McC	McCarthy (1960).
Merr50	Merrill and Burwell (1950).
MerSt76	Merrill and Stein (1976).
MGSJ97	Moody, Gregory, Soukup, and Jaderlund (1997
Mich	W. P. Bidelman and D. J. MacConnell, unpublished. The observations were made on 108 A/mm objective-prism plates taken with the University of Michigan's Schmidt telescope at Cerro Tololo
Mik78	Mikami (1978).
Mic97	Mickaelian (1997).
MSB	Merrill, Sanford, and Burwell (1933, 1942).
MSGAL85	Mould, Schneider, Gordon, Aaronson, and Liebert (1985).
Nass64	Nassau, Stephenson, and Caprioli (1964).
NassCam	Nassau and Cameron (1956). Cited only if the star did not later appear with a C number.
NassCol	Nassau and Colacevich (1950). The numerical C types quoted from this paper are defined in the paper; they essentially describe the CN strength, and the redness, of the spectrum in the infrared.
NassSte61	Nassau and Stephenson (1961).
NassvanAl	Nassau and van Albada (1949).
NETC	Nguyen-Q-Rieu, Epchtein, Truong-Bach, and Cohen (1987).
Nik	Nikolashvili (1987a).
Nik2	Nikolashvili (1987b).
Nik3	Nikolashvili (1987c).
NSV	New Catalogue of Suspected Variable Stars (Kukarkin et al., 1982).
OLFHHS	Omont, Loup, Forveille, Hekkert, Habing, and Sivagnanam (1993).
OrlRod74	Orlov, Rodriges (1974).
Perr59	Perraud and Pelletier (1959).
Perr61	Perraud (1961).
	Pesch, unpublished, Case objective-prism
Pes67	Pesch, (1967).
Phil67	Philip (1967).
Pick11	Pickering (1911).
Po78	Poulakos (1978).
Pots	The Potsdam Spektral-Durchmusterung (Becker 1931; Becker Bruck 1935-38).
Poul	Poulakos (1972).
Richt	Richter, Schaifers, and Wentzel (1961).
Ros51	Rosino (1951).
San49	Sanford (1949).
SandPhil	Sanduleak and Philip (1968).
Schai59	Schaifers (1959).
Schai60	Schaifers (1960).
SHLE96	Sarre, Hurst, and Lloyd Evans (1996).
Slet	Slettebak, Keenan, and Brundage (1969).
Smith37	Smith (1937).
Sndlk	N. Sanduleak, unpublished, various objective-prism plates taken at Cerro Tololo.
SndPes	Sanduleak and Pesch (1982).
SndPes88	Sanduleak and Pesch (1988).
Sop85	Sopka, Hildebrand, Jaffe, Gatley, Roellig, and Werner (1985).
SoyMae91	Soyano and Maehara (1991).
SoyMae93	Soyano and Maehara (1993).
Soymae99	Soyano and Maehara (1999).
Ste	Stephenson, unpublished, various objective-prism plates (Case, Hamburg, Bosscha, Cerro Tololo) unless slit spectrograms mentioned in the notes.
Ste65	Stephenson (1965).
Ste76	Stephenson (1976).
Ste85	Stephenson (1985).
Sto	Stock and Wroblewski (1972).
Thack49	Thackeray (1949).
The68	The (1968).
Tot98	Totten and Irwin (1998).
Upgr60	Upgren (1960).
Upgr68	Upgren and Grossenbacher (1968).
Van	Vandervoort (1958).
VB	V. Blanco, unpublished.
Vet	Vetesnik (1979).
VKL92	Volk, Kwok, and Langill (1992).
Vogt	Vogt (1973).
VyssBalz58	Vyssotsky and Balz (1958).
W	Westerlund (1971).
W58	Westerlund (1958).
W65	Westerlund (1965).
War65	Warner (1965).
War93	Warren, Irwin, Evans, Liebert, Osmer and Hewett (1993).
Wil73	Wilson, Schwartz, and Epstein (1973).
WMFCMC	Whitelock, Menzies, Feast, Catchpole, Marang, and Carter (1995).
Wray	Wray (1966). CE = H alpha emission.
WY77	Wing, Yorka (1977).

<<Except for the occurrence of the CCCS numbers, the ordering of the carbon star-finding lists under “designations” in Table 1 is generally the order in which I have become aware of them. The major exception is myself (Ste), whom I have usually listed last regardless of history. The overwhelming majority of these separately-found identifications for the same carbon star are, to the best of my knowledge - and certainly for my own surveys - completely independent rediscoveries.>>

n. <<Four symbols were introduced in the CCCS and are retained here. (1) An asterisk indicates that Table 1 equates two or more data in literal contradiction to one or more papers cited; for example, a much later paper may be reporting a new carbon star already so identified in a much earlier paper, which implies that perhaps there are two carbon stars in the area. This was a natural flag to use in the CCCS, where carbon stars were mainly reported in a few large and well-known surveys. It is no longer natural now, where the main pre-publication comparison has been with the CCCS, and there have meanwhile been many relatively short lists. Thus, I have added few if any new asterisks. Finally, a single asterisk meant that my fusing of two or more reports was based on coordinates alone, without any plate re-examination. In fact, many or most of these cases have now been routinely re-examined through later, systematic, surveys; but I have retained the asterisk to show the historical order. (2) A double asterisk means the same as a single one, except that I have specially re-examined plates with the identification problem in mind. As in (1), many of these have been further checked routinely by later, systematic surveys, where the finding of only one star allows the strong presumption that only one carbon star is involved. There are few or no new double asterisks in the present edition. (3) A plus sign signals a GCVS identification made by me by comparing an objective prism plate with a published identification chart. These, too, are mostly holdovers from the CCCS, because the host of more accurate coordinates for carbon stars in the present edition usually restricts any challenge to identifying a carbon star with a GCVS cool-giant variability type to the question (at least on deep plates): is there any other banded spectrum near the carbon star? (4) An R signals further remarks at the end of Table 1.>>

The object of the remarks is twofold. First, remarks are intended as an extension to the entries “Designations” and “Spectrum” of the catalog comprising matter for which there was no place in the Table. Second, remarks contain information about considerable disagreement in the position of a star determined by different authors or cases when there is some doubt if the data refer to the same star. We repeat Stephenson's remarks, although in a shortened form, in which he confirms discoveries or points to certain spectral and photometric peculiarities (outstanding spectral lines and bands, very red color etc.). Also we indicate the cases when a carbon star lies in the sky within boundaries of some star clusters and note conclusions about the membership, if possible. Also the stars with such distinguishing features as circumstellar silicate envelopes, detached gas and dust shells, maser emission, binarity and bipolar molecular outflows are marked.

P. Estimated precision class of the equatorial coordinates of the star: 0-1 for ±0.1 arcsec, 2 for ±1 arcsec and 3 for ±0.1 arcmin. Values of the precision class have been estimated by comparing coordinates of the stars determined by different authors. The highest precision class 0 was assigned only to the positions determined by Hipparcos, by MacConnell (2000) and for dwarf carbon stars.

3. REJECTED STARS

Table 2 contains 21 stars that have been declared as carbon or possible carbon stars but this classification was rejected in other publications. This table is a supplement to Table 2 in the 2nd edition of the Catalogue. The first five columns coincide with those in the Catalogue (Table 1), the 6th column gives the reference to the publication (with abbreviations of Section 2), the designation and the carbon spectral type, the 7th column gives the same for the publications in which this classification has been rejected.

Table 2.

Stars that have been published as carbon but probably or definitely are not.

RA(2000)	DEC(2000)	b	v	i	Designations or Sp. type	Remarks

00 30 30.0	+26 02 00		9.6		Crg61 (R)	K0 III (OrlRod74)
05 59 07.2	-10 52 38				HB75 (R)	S (WY77)
08 01 12.0	-36 27 00		9.8		Ros51 (Rp), AR Pup	F0-F8 (GCVS)
08 19 50.1	+37 27 32			16.5r	SndPes88=CLS 1(C:)	not C (GreMar90,Bot91)
08 22 28.2	+38 03 52			16.5r	SndPes88=CLS 3(C:)	not C (GreMar90,Bot91)
09 18 06.3	+29 04 10			13.0r	SndPes88=CLS 12(C:)	not C (GreMar90,Bot91)
09 59 32.4	+36 36 31			16.0r	SndPes88=CLS 20(C:)	not C (Bot91)
10 02 48.3	+30 56 47			16.0r	SndPes88=CLS 21(C:)	not C (Bot91)
11 11 27.4	+32 37 24			15.0r	SndPes88=CLS 35(C:)	not C (GreMar90)
13 51 16.4	+30 17 41			16.5r	SndPes88=CLS 75(C:)	not C (Bot91)
14 14 09.5	+32 32 32			16.0r	SndPes88=CLS 78(C:)	not C (Bot91)
15 02 37.2	+33 13 04			15.5r	SndPes88=CLS 85(C:)	not C (GMAC)
15 40 23.0	+34 29 47			15.0r	SndPes88=CLS 94(C:)	not C (GreMar94)
15 47 22.4	+31 45 18			17.0r	SndPes88=CLS 95(C:)	not C (GreMar94)
16 44 01.4	+33 41 18			16.0r	SndPes88=CLS 107(C:)	not C (GMAC)
16 45 53.8	+31 54 38			16.5r	SndPes88=CLS 108(C:)	not C (GreMar94)
18 32 42.3	-14 51 57				HB75 (R)	K5 (Bid80)
18 58 24.0	+04 39 56				HB75 (R)	M (Bid80)
19 13 11.7	+26 00 28		13.8		Soymae99 (C), S Lyr	S star (Ste76)
23 30 11.0	+60 16 47	18.9	14.8	12.0r	Po78 (C)	M (Bid80)
23 30 44.0	+60 15 32	16.2	12.1	9.2r	Po78 (C)	M (Bid80)

ACKNOWLEDGMENTS. We are grateful to Robert F. Wing, Chairman of the IAU Working Group on Peculiar Red Giant Stars for encouragement to start this work. We thank the authors who sent us reprints of their papers containing lists of carbon stars, especially, Hideo Maehara and Takao Soyano from the National Astronomical Observatory of Japan, Omar M.Kurtanidze and Maria G.Nikolashvili from Abastumani Astrophysical Observatory. We are thankful to D. Jack MacConnell from Space Telescope Science Institute (U.S.A.) who put at our disposal his unpublished list of new southern carbon stars and also pointed to the corrections needed for coordinates of several stars in the 2nd edition of the Catalogue. We are also thankful to William Buscombe from Northwestern University (U.S.A.) for supplying us with his latest catalogs of MK Spectral Classification. Our work has been supported by the grant No.96.0225 from the Latvian Council of Science.

References

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Abramyan G.V., Gigoyan K.S. 1990, Astrofizika, 32, 501

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PART II. REMARKS

0001+6021	5976	+59°2810, C 29, Har (Np), Ste, MaeSoy 37, BDS 12693, AFGL 3196, IRC+60433. San: N; K-M: C9,1; Yam: C9,2JLi; KB: SC6-8/10e. WZ Cas has long been famous for the outstanding strength of LiI 6707 Å line, and also for the strength of the sodium D lines. The star is extremely red, and in I magnitude it is one of the brightest carbon stars in the sky. See also Bidelman (1954).
0002-0249	5980	D 156(K), Van(R2). San: R0. A CH star (Bidelman 1956), Yam(C1,1CH). Spectroscopic binary with a period of 1273 days.
0002+5958	5981	Also MaeSoy 41.
0002+6337	5983	Also Nik 27.
0004+6418	5985	Also MaeSoy 43, VB 8023-28.
0004+6055	5986	Also MaeSoy 44.
0004+4333	5987	+42°4827, BSD 43-504 (Nb), D 365 (R), AFGL 11, IRC+40003, Ste (N, two surveys). Visual companion: V = 12.77 mag, F0V, 15² away.
0007+6148	9	Nik 31.
0007+6443	8	Also Nik 30, Ste
0011+6429	12	Nik 32
0013+6327	19	+62°25, MaeSoy 58. Published as R2 by San, but has strong D lines.
0015+6312	26	Nik 36.
0017+1052	31	Weak C₂.
0017+5017	32	D 235 (R), C 694, Ste (N).
0019+4442	36	+43°53, D 236 (N), C 695, Ste. San: N; Yam: J star.
0020+6029	37	Nik 38, Ste.
0021+5914	41	Also Ste, MaeSoy 69.
0022+5911	43	C 521, Poul, MaeSoy 71, Ste.
0024+6142	47	Nik 40.
0024+5417	53	+53°66, C 696, Van 1 (R5). Yam: C4,5J.
0026+6118	57	Nik 45, Ste.
0027+3535	65	D 157 (N), Ste (N), AFGL 68, IRC+40010.
0035+7031	83	AFGL 86S, IRC+70009.
0035+6119	82	MaeSoy 91, CCCS 20.
0035+5800	86	Also MaeSoy 93, Ste.
0035+6037	89	Also Ste.
0039+6046	97	MaeSoy 97, Ste.
0041+6128	100	Nik 53.
0041-2619	102	Sanduleak and Philip (1968): probable early R, from color.
0042+6328	101	Also Ste.
0046+5937	111	Also Ste.
0050+6317	121	MaeSoy 97.
0050-1904	124	Also BidMac. Weak C₂, but fairly strong red CN (Ste).
0052+6019	127	MaeSoy 110, Ste. Case plates suggest variable (Ste).
0052+6011	128	MaeSoy 111. Not the nearby 0052+6019.
0053+6320	131	VB 8024-30, MaeSoy 113.
0054+2404	135	+23°123, Van 98 (R), Ste (R). A CH star (K-M, Yam(C1,2)). Spectroscopic binary with a period of 755 days.
0054+5833	136	+57°165, AFGL 4062S, IRC+60026, Ste, MaeSoy 115. A CS star (Ste); cf. Keenan (1950). Yam: C7,1e.
0054+5923	134	Large radial velocity (-232 km/s) and proper motion (0.149’‘/yr).
0056+6427	143	MaeSoy 118.
0059+6348	149	MaeSoy 120.
0059+6044	150	VB 8024-42, MaeSoy 121.
0059+3920	154	C₂ weak.
0100+6020	157	C₂ weak.
0100+6216	160	Nik 67, Ste.
0102+6151	165	Har, Ste, Kurt78 8, MaeSoy 127, AFGL 146S, IRC+60034.
0104+6122	167	MaeSoy 128.
0109-2821	177	Also Slet, CCCS 55.
0110+6154	176	Also Ste.
0111+5341	180	Yam: C4,3e.
0112+6211	185	Also Ste, Nik77. 2¢ position difference with V418 Cas, which is not a carbon star.
0112+6022	187	MaeSoy 141.
0113+5951	188	MaeSoy 142, IRC+60041, CCCS 58.
0113+6257	189	MaeSoy 143.
0116+5738	197	Variable, 13.2-13.8 (BC).
0116+2546	198	D 159 (N), Ste (N), AFGL 188, IRC+30025. Yam: C7,2.
0117+6713	6017	also OLFHHS, VKL92, AFGL 190.
0118+6252	204	MaeSoy 151.
0118+5809	205	CCCS 65. In area of the open cluster NGC 103.
0126-3232	234	-33°525, AFGL 215, IRC-30015, Slet (N=C5,4, SiC₂), Hen. San: Np; Yam: C6,4. The star has a detached gas shell.
0128+6216	233	Also MaeSoy 167.
0129+5853	235	Also MaeSoy 168.
0133+5745	238	D 243(N), C 530, MaeSoy 170, AFGL 6161S, IRC+60056. Yam: C5,5.
0134+5743	239	Probably NSV 547 (Bidun).
0140-1856	256	Also BidMac.
0142+6305	253	MaeSoy 179.
0142+6336	255	MaeSoy 181.
0145+5357	268	D 244 (R), Van (R5), Har (ER), CCCS 82. Yam: C3,5JCH.
0152+5658	289	In area of the open cluster Stock 4.
0156+5915	295	+58°334a, Ste, MaeSoy 201 AFGL 270S, IRC+60069. Yam: C5,4e.
0156+5918	296	MaeSoy 202.
0158+5512	297	Ha emission star No. 658 in Publ. Vat. Obs. 1, No. 12.
0201+5750	305	MaeSoy 206.
0201+5818	303	CCCS 90.
0202+6106	306	Also Nik3 2.
0206+5650	310	Also Ste, two surveys. Ha emission reported by Bidelman (1965).
0214+4739	324	May be S, not C. Very strong D lines.
0215+1214	327	D 1 (R), Van 5 (R8), Ste. A CH star (K-M, Yam(C4,4)).
0215+6416	325	The quoted RA is by 16 s greater than Kurtun and DEC is by 1¢ smaller (Ste).
0216+6253	326	Also Nik3 13, Ste.
0221+6004	339	Also Bidelman, SoyMae91.
0225-1323	353	-14°450 (BidMac).
0226+5207	350	D 248 (N), IRC+50061. Yam: C5,5.
0227+5859	352	Also SoyMae91.
0228-0721	357	Yam: C4:,0+.
0229-2605	361	Hanbl, IRC-30021. See also Sanford (1944).
0232+5814	365	CCCS 105. The identification of the carbon star with the variable can be made from the charts published for each.
0232+5951	364	Also SoyMae91. Identical with CCGCS 362.
0233+5802	6034	Also GWSK, VKL92, AFGL 341.
0235+5608	372	A 6168 star (De). Yam: C4,5.
0235-0926	378	-10°513, Ste (R). San: R4; Yam: C2,3J.
0238+5545	384	D 250 (R), C 544, Har (LR), Ste. Yam: C4,5J.
0238+3910	387	+38°525, D 160 (R). Yam: C5,4.
0240+6216	388	Also SoyMae91.
0244+6018	398	The quoted position is from an infrared Case plate (Ste).
0246+4707	403	BSD 22-3484 (NA), Ste (N:).
0250+5853	409	SoyMae position is used which differs by 1¢ in DEC from Ste.
0252+3828	417	Probably V448 Per = NSV 966 (Bidun).
0253+5957	415	SoyMae position is used which differs by about 1.5¢ in DEC from Ste.
0311+5754	451	D 255 (R), C 2, Van 8 (R5), Har (ER), Ste, SoyMae91, AFGL 453, IRC+60113, CCCS 131. San: R6; Yam: C4,5J.
0313+4749	461	D 256 (R), Har (EN), Ste, IRC+50088, CCCS 134. Yam: C7,4.
0312-5719	471	HR 977, -57°626, Hen.
0316+5823	467	Also SoyMae91. Dean: C5,3.
0316-2810	478	-28°1082 (BidMac).
0318+6128	473	Also SoyMae91.
0324+6035	489	Also SoyMae91.
0326+4731	496	Also SoyMae91, AFGL 489, IRC+50096.
0327+4410	500	+43°726, D 260(R), Van 9. Yam: C5,3e.
0328+2040	503	IRAS spectral tracing confirms carbon star.
0332+5244	514	Also SoyMae91. In area of the open cluster Berk 9.
0332+4126	515	CCCS 149.
0339+6141	531	The SoyMae91 position is given.
0340+5905	534	The SoyMae91 position is given; the Nik3 RA is about 7^s smaller and DEC is 15² smaller.
0340+6105	535	The SoyMae91 position is given.
0341+6238	540	+62°596, D 264 (N), C 697, Har (N6), Ste (N), IRC+60124. SiC₂ bands. Also San: N. The star has two detached gas shells.
0341+5130	541	+51°762, D 265 (N), MSB 3 (N), Har (LN), Ste (N), SoyMae91.
0345+5621	553	The SoyMae91 positon is given. NSV 1253 according to the Case paper.
0345+5355	555	Assumed to be Nik4 13, received with no minutes of declination. The quoted position is from two accordant Ste survey plates.
0345+4446	556	D 266 (N), Ste (N), IRC+40067.
0346+5139	559	Also BidMac.
0350-4332	576	Pots 167-194 (R4), Hen 3.
0352+3951	572	IRC+40070. Revised coordinates. The position of the variable is 2¢ away. GJBSW identify it with IRAS 03488+3934.
0353+5043	574	The SoyMae91 position is given.
0356+4348	578	C 551, Har(LR or N), Ste(N).
0358+1154	588	Also Ste(R). NSV 1426. Yam: C4,3.
0400+5844	583	The SoyMae91 position is given; the Case RA is about 6^s smaller and DEC is 1¢ larger.
0400+2332	594	Yam: C3,3J.
0403+5613	599	CCCS 174
0403+5541	600	The SoyMae91 position is given; the Nik4 RA is 8^s larger and DEC is 45 larger.
0404+2314	610	Yam: C3,0CH.
0405+6147	608	+61°667, D 272 (R), Van 13 (R8), Ste, AFGL 4316S, IRC+60138. K-M: C5,3; Yam: C5,4J. HD: a typical R8 star.
0408+6127	614	Also MacCon.
0410+5126	619	The SoyMae position is used which differs by about 1¢ in DEC from Ste.
0410+4426	622	NSV 1481.
0411+5119	623	C 4, Ste (N), SoyMae91.
0412+5109	625	CCCS 184.
0415+5255	634	+52°790, BC 190, a Dearborn M star, is about 5¢ away, and IRC+50112 is midway between both, hence probably is blended by both stars.
0416+5037	643	C 5, Ste (N), SoyMae91, AFGL 558, IRC+50115. Strong SiC₂. Yam: C6,4. See also Bidelman (1954).
0417+0653	657	Bidun finds the C₂ bands, if present, to be very weak. Never picked up on any Case survey. Dean, from the visual region, classified it as K5.
0418+2621	654	Formerly identified with BO Tau, now considered to be of RR Lyrae-type.
0419+4710	653	Also SoyMae91. Strong D lines (Ste).
0419+4107	659	C 559, Har, Ste.
0425+5256	680	Also SoyMae91.
0425+5014	679	Also SoyMae91. The C 73 published DEC was 1° in error.
0426+5146	682	CCCS 210
0426+5012	681	Also SoyMae91. C 74 had its published DEC misprinted by 1°.
0428+2531	696	CCCS 213.
0429+3952	701	D 166 (N), C 561, AFGL 582, IRC+40089.
0430-6559	725	Noted in HD as perhaps intermediate between classes K and R.
0431+4514	707	Strong SiC₂ bands (Ste).
0431+1739	714	Spectrum Ne quoted by Luyten and Merrill (1954).
0439+4137	737	C 78, Ste(N).
0442+3606	6086	May be protoplanetary nebula in the process of formation (GCVS).
0445-3131	777	Also BidMac.
0447-3612	788	-36°1884, Hen 5. Yam: C6,3.
0448+4418	771	Very weak C₂.
0449+3958	780	An LS V OB lies near the same declination and 1.4^s E of the carbon star. The two stars are of similar brightness on the infrared plate (Ste).
0449+3500	781	D 171 (R), C 504, Van 15 (R8), Har (ER), Ste. Yam: C4,3CH. Spectroscopic binary with a period of 2954 days.
0450+1547	793	D 6 (N), C 699, Ste, CCCS 253.
0451+6810	769	+67°350, D 275 (N), C 698, Ste, AFGL 633, IRC+70055. HD: a typical star of class Nb; K-M: C5,4.
0451+4340	789	In area of the cluster NGC 1664, nonmember by proper motion.
0451+2831	794	+28°707, D 172 (N), Har (N), Ste, MaeSoy2 2, AFGL 639, IRC+30098. GCVS: C4,2-C7,4.
0452+3830	797	Also Ste (CS, probably weak C), AFGL 643, IRC+40101, CCCS 257. Yam: C8,1J.
0453+4957	803	AFGL 4385S, IRC+50130.
0453+4041	805	The identification chart published by the Gonzaleses (1956) plus a Case plate show that this is their Ha-emission star No. 306. The spectrum shows SiC₂ bands (Ste). The quoted position is from two accordant plates of the Ste infrared survey.
0453+2246	808	MaeSoy2 4.
0454+4954	806	D 276(R), C 329, Ste (N).
0455+4150	814	Not the nearby 0455+4152.
0457+3207	819	V336 Aur, MaeSoy2 7.
0458+1654	826	Noted by Luyten (1956) as a very red star.
0459+0807	828	+7°768, D 9, Ste. KB: SC6/10e; Yam: C8,1e. See also Bidelman (1954).
0459-1448	833	HD 31996 (Pec), -15°915, Ste (N), IRC-10080. K-M: C7,4+; Yam: C7,4e. See also Bidelman (1954). HD: like VX And.
0500+4548	827	A weak CS star, with no certain C₂. Possibly an S star. Published as a reddened early M (therefore a presumed supergiant) by Nassau and Blanco (1957), their No. 116.
0503+5037	836	+50°1112, D 277 (N), Har (N), AFGL 672, IRC+50135. Yam: C5,4.
0503+4218	839	Also Fuen 3.
0505+0110	853	+0°939, D 12 (N), Ste (N), AFGL 683, IRC+00066. San: N; K-M: C5,3. See also Bidelman (1954).
0509+3900	860	+38°1035, D 173(N), C 7, Har(N), Ste, Fuen 7, IRC+40115. Yam: C5,4.
0509+2954	864	MaeSoy2 11.
0509-0530	875	-5°1174, Ste (N), IRC-10083. San: N.
0510+3923	866	CCCS 293.
0510+3949	867	CCCS 292.
0511+2938	874	MaeSoy2 13.
0511+1450	876	Missing from the longer Dearborn list, but according Ste the Case plates definitely confirm this star in this position. Dean: C6:,9.
0512+1453	879	Present in the early short list of the Dearborn carbon stars but not in the later longer list of red stars; but the Case plates confirm the carbon star (Ste).
0514+3447	883	Also Fuen 14, Ste.
0515+1158	893	+11°755, Ste (N), Epc90-6, IRC+10081.
0517+2741	896	Also Fuen 21, MaeSoy2 15.
0517+3212	899	MaeSoy2 16, Ste.
0517-7110	931	Very weak C₂ (Ste, Sndlk). Within 2° of a similar star, HD 36598. In the Large Magellanic Cloud field; Fehrenbach reports high velocity.
0518+3515	900	Also Fuen 23, Ste.
0519+3547	904	D 178 (N), C 8, Har (EN), Upgr68, Ste, Fuen 25, AFGL 4401S, IRC+40120. San: N. Visual companion V = 13.43 mag, 24² away.
0521+3723	910	Also Fuen 28.
0521+3230	911	+32°957, D 179 (R?), C 9, Upgr68, Ste (N), Fuen 29, MaeSoy2 18, AFGL 735, IRC+30110. ADS 3934A, 3.5² in PA 4°. SiC₂ (Merrill 1926). The only known carbon star whose spectrum shows NeIII and OIII, cf. Sanford (1950b). See also Gordon (1968) and Bidelman (1954).
0521+0721	914	NSV 1941, BidMac, IRC+10083, CCCS 319. Yam: C4:,4.
0523+3228	917	MaeSoy2 20.
0524+3432	921	Fuenmayor's position, given here, differs by 1 min in RA from Upgr68, but is supported by a computer overlay.
0524+3032	923	Also Fuen 36, MaeSoy2 23.
0525+4908	925	The Dearborn position, quoted here, has been checked by a computer overlay.
0525+3349	926	Also Fuen 38.
0526+3224	936	Upgr68, Ste, Fuen 45, MaeSoy2 25.
0526+2402	938	MaeSoy2 26.
0526+3200	939	Also Ste, MaeSoy2 27.
0526-7004	984	About 2° from a similar weak-C₂ star, HDE 269343. A BaII star according to MacConnell et al. (1972).
0527+3408	941	+34°1044, C 10, Upgr68, Ste, Fuen 49, AFGL 748, IRC+30114.
0528+3430	946	Also Fuen 51, Ste.
0528+3529	948	Also Ste.
0529+4324	950	+43°1278, D 280 (R), C 272, Ste (N). San: N; Yam: C5,4.
0529+0329	958	Also Ste (N).
0530+3159	956	MaeSoy2 29, Ste.
0530+3143	959	MaeSoy2 30, Ste.
0531+3439	961	Ste, Fuen 63.
0531+3154	962	Ste, Fuen 64, MaeSoy2 31.
0531+2816	964	MaeSoy2 33.
0531+2333	965	MaeSoy2 32.
0532+2931	966	MaeSoy2 34.
0532+2940	971	MaeSoy2 35.
0532+3256	972	Upgr68, Ste, Fuen 71, MaeSoy2 36.
0532+2829	973	MaeSoy2 37.
0532+1544	977	De: C5,3.
0533+3211	976	MaeSoy2 38.
0533+3320	981	Also Ste.
0533+0709	988	+7°929, D 22 (N), Ste (N), IRC+10089.
0534+2451	990	D181 (R), C 505, Dol62, Ste, Fuen 78, MaeSoy2 42. Har: ER.
0535+3351	991	Ste, Fuen 79.
0535-2543	1004	-25°2539, Van 17 (R8), Sto III-1(N), Hen 7, AFGL 4429S, IRC-30046. Yam: C6,4. According to Hipparcos data, periodic N-type variable with the shortest known period of 82.7 days.
0537+3003	1003	MaeSoy2 46.
0538+2249	1006	MaeSoy2 47.
0538+3026	1008	MaeSoy2 48.
0539-0807	1017	Also IRC-10095, Epc90-9, AFGL 796. 2¢ position difference with GCVS.
0539+3326	1009	Also Fuen 86.
0540+4919	1007	C₂ is not reached on the Ste plate, but very strong CN.
0541+6847	998	+68°398, D 281 (N), Van 16, IRC+70064; see also Bidelman (1954). San: R8e; Yam: C7,2Je.
0541+3437	1014	Also Ste.
0541+1217	1022	Also Epc90-10, IRC+10094. Possibly NSV 2557, although a Haro Ha-emission object is also nearby (but different from the carbon star). The Dearborn position has been slightly improved with the aid of a Case plate and a computer underlay.
0542+2817	1025	MaeSoy2 53.
0542-1646	1035	Yam: C2:,0+.
0543+3340	1026	Also Fuen 95.
0543+1004	1031	De: C6,3.
0543-4627	1052	The spectral type in Pickering (1911) appears to be due to Mrs. Fleming. Bidun has noted SiC₂ in the spectrum.
0545+2425	1038	+24°943, D 183 (N), C 11, Van (C:), Ste (N:), Har (N), Fuen 100, MaeSoy2 57, AFGL 390, IRC+20120. Spectrum composite, see Gordon (1968). Sanford: N. Spectroscopic binary.
0545+2529	1041	MaeSoy2 58.
0545+2041	1042	+20°1083, D 30 (N), C 507, Van (N), Ste, Har (EN). San: N; Bid: C7,4e; Yam: C6,4.
0545+1530	1043	+15°921, MSB 13 (N), D 31 (R), C 508, Ste (N). Yam:C5,4.
0545+1216	1044	AFGL 393, IRC+20121. Very strong D lines.
0546+2538	1049	MaeSoy2 61.
0547+2851	1053	Also Fuen 105, MaeSoy2 63.
0547+3034	1058	MaeSoy2 65.
0548+4454	1057	MSB 14, D 285 (N), IRC+40141.
0548+3037	1061	+30°1014, D 184 (N), C 273, Har (LR pec), Ste (R-N), Fuen 110, MaeSoy2 67. San: N.
0548+2613	1067	MaeSoy2 69.
0549+3202	1068	MaeSoy2 70.
0549+1904	6106	Spectral class from GCVS.
0550+2517	1078	MaeSoy2 73.
0550+2216	1079	MaeSoy2 74. In area of the open cluster Berk 72.
0550-0203	1086	Letter from Boeshaar to Bidelman: V-I = 3.7 mag.
0552+3211	1088	Ste , Fuen 122, MaeSoy2 76.
0552+2954	1089	NSV 2684, Fuen 123, MaeSoy2 77.
0552+2950	1090	MaeSoy2 78.
0553+3038	1092	MaeSoy2 79.
0554+2838	1096	Also MaeSoy2 84.
0554+0105	1101	Also BidMac.
0554+3011	1098	MaeSoy2 86.
0554-8403	1212	Mayall (1951) identifies with CPD -84°86.
0555+3127	1099	Fuen 133, MaeSoy2 87. BN Aur is about 5¢ distant from this C star.
0555+3402	1100	Also Fuen 134.
0555+3202	1103	Also MaeSoy2 89. CS type in the red spectral region, but enough infrared CN to be called carbon by Nassau-Blanco, Fuen, MaeSoy, and Ste. AY Aur is nearby and seen separately (on the red and infrared objective prism plates) as an M star.
0556+3352	1104	Har: LR.
0556+3006	1109	NSV 2735, MaeSoy2 93, Ste.

Electronic Version 2001.1 at 2001-06-21

Third Edition

A.Alksnis, A.Balklavs, U.Dzervitis, I.Eglitis, O.Paupers and I.Pundure