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\begin{document}

\IBVShead{5185}{12 October 2001}

\IBVStitletl{Coordinates and Identifications for}{ Dolidze S, C, and MS Stars}

\IBVSauth{Skiff, Brian A.}

\IBVSinsto{Lowell Observatory, 1400 West Mars Hill Road, Flagstaff\enskip AZ\enskip 86001-4499, USA\enskip (bas@lowell.edu)} %email


\begintext

In the course of other work I have obtained complete identifications
for a problematic list of late-type stars by Dolidze (1975a).  The
charts were used to make the identifications.  Since numerous
substantial errors were found that have propagated elsewhere in the
literature, it was thought useful to publish the list separately.  The
corrections allow linkage of the stars to other catalogues in the
visible and infrared.  This complements a second similar list of late-M
stars by Dolidze (Dolidze 1975b, Skiff 1997).

Table 1 lists the ninety-one stars along with the best available
positions and principal identifications.  The acronym `[D75b] Star' has
been assigned to the stars in the Lortet {\it et al.}\ (1994)
``Dictionary''.  An asterisk next to the name indicates a note
following the table.  The coordinates were drawn, in descending order
of preference, from:  UCAC1 (Zacharias {\it et al.}\ 2000), Tycho-2
(H{\o}g {\it et al.}\ 2000), the 2MASS point-source catalogue (second
release, Skrutskie {\it et al.}\ 2000), GSC-ACT (Gray 1999), USNO-A2.0
(Monet {\it et al.}\ 1998), or the recent GSC-2.2 (STScI 2001).  The
source of the positions is coded in column `s' as follows:  A =
USNO-A2.0, G = GSC-ACT, g = GSC-2.2, M = 2MASS, T = Tycho-2, U =
UCAC1.

GSC and IRAS names are given as available.  The MSX catalogue (Price
{\it et al.}\ 2001) was a useful aid in identifying some of the stars.
MSX identifications are shown in the notes for objects not appearing in
the IRAS catalogue.  Since no indication of brightness is given for the
stars by Dolidze (or in SIMBAD), rough photo-blue magnitudes largely
from USNO-A2.0 are listed for nearly all the stars.  The spectral types
are from Dolidze.  As indicated in the notes, not all of these are
correct, but are given as a record of the source paper.  The last
column shows mostly variable-star designations or names from the
Stephenson S-star (1984, CSS) and carbon-star (1989, CGCS) or
``reddened'' star (Stephenson 1992, StRS) catalogues.  Two-thirds of
the stars have additional identifications and comments in the notes.

\normalsize
\begin{center}
{Table 1:  Positions and identifications} \\
\begin{tabular}{lrlccclll}
\hline
[D75b] & \multicolumn{2}{c}{RA\quad (2000)\quad Dec}& s & GSC & IRAS & mb & spec & Other IDs \\
\hline
~\,1*& 0 07 42.6~\,& +60 22 54   &-& 4014-0240 &            & 15.1 & S    & CSS 4 \\
~\,2 &  0 46 53.27 & +56 40 08.4 &G& 3663-1363 & 00439+5623 &      & C    & GW Cas \\
~\,3 &  1 00 53.16 & +56 36 45.2 &T& 3676-1346 & 00578+5620 & 10.9 & S7,2 & V365 Cas \\
~\,4 &  1 28 36.19 & +61 12 07.7 &G& 4031-2015 & 01252+6056 &      & S    & PQ Cas \\
~\,5 &  1 29 44.00 & +61 41 41.7 &G& 4031-1549 & 01263+6125 & 15.2 & S    & CSS 37 \\
~\,6*&  1 35 09.71 & +60 17 09.9 &G& 4031-2130 & 01318+6001 & 15.5 & S    & CSS 38 \\
~\,7*&  1 54 19.71 & +21 53 20.6 &T& 1212-0468 & 01515+2138 & 10.6 & S7,3 & NSV 15403 \\
\hline
\end{tabular}
\end{center}
\vfil
\eject

\begin{center}
{Table 1 (cont'd.):  Positions and identifications} \\
\begin{tabular}{lrlccclll}
\hline
[D75b] & \multicolumn{2}{c}{RA\quad (2000)\quad Dec}& s & GSC & IRAS & mb & spec & Other IDs \\
\hline
~\,8 &  2 08 31.02 & +62 22 44.5 &G& 4037-2533 & 02048+6208 & 14.4 & S    & CSS 47 \\
~\,9 &  2 18 52.44 & +62 48 13.5 &G& 4050-0812 & 02151+6234 & 18.2 & S    & CSS 50 \\
10  &  2 19 16.76 & +59 42 21.5 &G& 3698-2179 & 02156+5928 & 15.1 & MS   & CSS 53 \\
11* &  2 21 20.28 & +61 23 54.0 &A&           & 02176+6110 & 19.1 & CS:  & CSS2 9 \\
12* &  2 23 11.95 & +63 51 58.1 &G& 4054-0897 &            & 17.1 & S    & StRS 44 \\
13  &  2 24 44.77 & +55 35 45.8 &A&           &            & 15.0 & MS   &  \\
14* &  2 25 19.32 & +58 16 10.4 &G& 3698-2696 &            & 16.0 & MS   &  \\
15  &  2 32 45.05 & +58 14 37.5 &G& 3699-1448 & 02290+5801 &      & C    & DU Per \\
16* &  2 38 33.45 & +61 54 31.1 &G& 4051-2337 &            & 15.6 & MS   & CSS 59 \\
17  &  2 40 29.35 & +62 16 20.3 &G& 4051-2343 & 02365+6203 & 15   & C    & CGCS 388 \\
18* &  2 44 31.02 & +60 18 49.6 &G& 4047-2083 &            & 16.8 & C    &  \\
19  &  2 46 23.19 & +60 08 20.0 &G& 4047-0252 & 02424+5955 & 16.3 & S    & CSS 64 \\
20  &  2 51 36.05 & +59 07 11.7 &A&           & 02478+5854 & 17.2 & S    & CSS 66 \\
21* &  2 53 44.55 & +58 57 44.1 &G& 3713-1162 & 02498+5845 & 15.7 & S    &  \\
22* &  2 58 14.89 & +61 43 07.2 &A&           &            & 16.2 & S    & CSS 68 \\
23* &  3 16 40.87 & +58 23 53.4 &G& 3714-0995 & 03127+5812 & 15.3 & C:   & CGCS 467 \\
24* &  3 17 36.46 & +59 41 52.3 &A&           & 03136+5930 & 17.7 & S    & CGCS 469 \\
25* &  3 39 50.79 & +51 06 30.6 &T& 3325-0367 & 03361+5056 & 13.3 & S    & CSS 78 \\
26* &  4 28 18.53 & +25 31 41.1 &G& 1833-0749 & 04252+2525 & 14.5 & C(R) & V414 Tau \\
27* &  4 56 07.33 & +48 03 05.8 &G& 3348-2323 &            & 15.5 & C:S: &  \\
28* &  4 59 15.25 & +47 36 01.2 &G& 3348-0978 & 04554+4731 & 15.9 & MS   &  \\
29* &  5 06 30.15 & +34 37 41.0 &G& 2397-0721 &            & 15.1 & S    & DK Aur \\
30* &  5 11 33.59 & +47 40 47.0 &G& 3349-0826 &            & 15.1 & MS   & CSS 122 \\
31  &  5 11 39.28 & +29 06 21.4 &G& 1858-0893 & 05085+2902 & 16.1 & S    & CSS 125 \\
32* &  5 25 29.98 & +32 53 08.3 &M& 2407-0897 &            & 14.6 & MS   & CSS 136 \\
33* &  5 28 37.35 & +34 02 28.1 &M& 2411-2106 &            & 15.2 & MS   & CSS 140 \\
34* &  5 29 33.67 & +27 49 34.2 &M& 1856-0659 &            & 14.3 & MS   &  \\
35  &  5 32 44.19 & +29 02 51.7 &M& 1860-0128 & 05295+2900 & 16.8 & MS   & CSS 143 \\
36  &  5 35 11.21 & +37 45 46.0 &M& 2910-0836 & 05318+3743 & 17.1 & MS   &  \\
37  &  5 36 52.06 & +29 02 15.4 &M&           & 05336+2900 & 17.8 & S    & CSS 146 \\
38* &  5 38 17.62 & +28 11 44.1 &M& 1873-0803 & 05350+2809 & 14.7 & S    & CSS 148 \\
39  &  5 38 22.19 & +35 37 29.2 &G& 2412-0264 & 05350+3535 & 16.1 & S    & CSS 147 \\
40* &  5 39 15.52 & +20 28 55.3 &M&           &            & 14.9 & S:C: &  \\
41* &  5 53 10.07 & +29 13 27.9 &M& 1875-0733 &            & 14.9 & S    & CSS 169 \\
42  &  6 02 37.80 & +29 07 05.8 &M& 1876-1740 &            & 15.1 & MS   & CSS 180 \\
43  &  6 05 27.89 & +22 20 42.1 &M&           & 06024+2220 & 15.7 & MS   & CSS 185 \\
44  &  6 08 26.23 & +28 06 43.1 &M& 1885-1055 & 06052+2807 & 13.9 & S    & CSS 188 \\
45  &  6 08 44.67 & +31 09 41.1 &M& 2419-1008 & 06054+3110 & 15.0 & S    & CSS 189 \\
46* &  6 09 32.97 & +31 31 46.6 &M&           & 06062+3132 & 14.9 & MS   & CSS 190 \\
47* &  6 10 09.60 & +23 33 00.9 &M&           &            & 14.7 & MS:  & CSS 193 \\
48  &  6 10 34.60 & +23 38 54.4 &M& 1877-1613 & 06075+2339 & 13.9 & MS:  & CSS 195 \\
49* &  6 18 52.52 & +21 12 16.1 &M& 1327-1382 &            & 15.2 & MS:  & CSS 208 \\
50  &  6 23 52.89 & +21 18 30.1 &T& 1327-1623 & 06208+2120 & 13.4 & S    & CSS 214 \\
51  &  6 36 27.03 & +07 00 33.3 &G& 0158-0371 & 06337+0703 & 14.9 & S    & CSS 232 \\
52* &  6 39 03.23 & +02 34 00.2 &A&           &            & 15.2 & MS   & CSS 240 \\
53  &  6 43 56.34 & +01 44 59.3 &A&           & 06413+0148 & 14.9 & S    & CSS 249 \\
54* &  6 44 42.71 & +07 03 58.2 &G& 0159-3098 &            & 15   & S    & CSS 250 \\
55* &  6 44 29.74 &$-$02 32 32.0&M& 4803-1048 &06419$-$0229& 14.2 & S    & NSV 3190 \\
56  &  6 45 32.39 & +06 47 06.4 &G& 0160-2107 &            & 15.1 & S    & CSS 255 \\
57  &  6 47 36.24 & +09 38 19.6 &G& 075102499 & 06448+0941 & 15.3 & MS   & BF Mon \\
58  &  6 48 08.67 & +06 29 24.1 &A&           & 06454+0632 & 15.6 & S    & CSS 259 \\
59  &  6 48 57.08 & +06 56 33.2 &G& 0160-0959 & 06462+0659 & 14.0 & S    & CSS 262 \\
60  &  6 55 40.14 &$-$05 31 02.4&G& 4809-0418 &06532$-$0527& 14.4 & S    & EN Mon \\
61* &  7 14 01.66 &$-$14 36 00.7&T& 5406-0728 &07117$-$1430& 12.8 & C5,2 & NSV 3471 \\
62* &  7 23 08.35 &$-$14 16 15.0&G& 5407-2172 &07208$-$1410& 16.0 & C3,3 & CGCS 1684 \\
\hline
\end{tabular}
\end{center}
\vfil
\eject

\begin{center}
{Table 1 (cont'd.):  Positions and identifications} \\
\begin{tabular}{lrlccclll}
\hline
[D75b] & \multicolumn{2}{c}{RA\quad (2000)\quad Dec}& s & GSC & IRAS & mb & spec & Other IDs \\
\hline
63* & 16 08 54.56 &$-$21 56 18.9&U& 6213-1036 &            & 14.7 & C:S: &  \\
64  & 18 22 42.51 &$-$16 29 28.2&U&           &18198$-$1631& 16.8 & S:C: & CSS 1035 \\
65* & 18 23 34.97 &$-$17 05 10.2&U& 6269-0443 &            & 12.8 & S    & CSS 1036 \\
66  & 18 33 02.93 &$-$19 46 26.1&G& 6275-0751 &18300$-$1948& 13.3 & S    & V2003 Sgr \\
67  & 18 30 34.57 & +36 14 57.0 &T& 2636-0435 & 18288+3612 &~\,9.3& M7Se & V530 Lyr \\
68* & 20 06 33.96 & +24 26 00.0 &T& 2158-0309 & 20044+2417 & 13.7 & S4,2 & DK Vul \\
69* & 20 09 10.39 & +21 57 03.1 &T& 1630-2890 & 20069+2148 & 12.4 & C2,5 & NSV 12842 \\
70  & 20 12 32.28 & +46 51 13.7 &G& 3559-2601 & 20109+4642 & 15.3 & S    & CSS 1197 \\
71  & 20 13 08.46 & +48 34 45.0 &T& 3563-0623 & 20116+4825 & 14.1 & C    & V1955 Cyg \\
72* & 20 27 08.12 & +36 33 06.5 &T& 2697-0092 & 20252+3623 & 13.2 & S    & V441 Cyg \\
73* & 20 28 06.44 & +42 55 07.2 &M&           & 20263+4245 & 18   & C    & CGCS 4868 \\
74  & 20 41 28.71 & +36 35 02.5 &M&           & 20395+3624 & 16.8 & C    & CGCS 4936 \\
75* & 20 45 55.29 & +36 32 18.6 &M& 2699-2004 &            & 15   & S    & CSS 1238 \\
76* & 20 47 43.36 & +34 19 03.3 &M& 2695-3678 & 20457+3408 & 15.8 & S    & V1976 Cyg \\
77* & 20 49 46.16 & +11 29 41.7 &T& 1098-1282 & 20473+1118 &~\,8.4& K2p  & HD 198403 \\
78* & 20 50 41.32 & +39 49 41.3 &A&           &            & 17.4 & S    & NSV 25365 \\
79* & 21 01 19.71 & +36 25 53.8 &M&           &            & 14.4 & S    & V1896 Cyg \\
80* & 21 14 19.81 & +38 00 58.5 &M&           &            & 18.8 & SC:  & V1235 Cyg \\
81* & 21 37 19.03 & +47 59 59.1 &M&           &            & 17.0 & S    & CSS 1280 \\
82* & 21 44 29.21 & +50 57 16.8 &A&           &            & 16.2 & S    & CSS 1282 \\
83* & 21 55 24.87 & +63 53 21.4 &G& 4270-0794 & 21540+6339 & 14.8 & C    & CGCS 5508 \\
84* & 22 04 06.10 & +59 52 45.2 &G& 3981-1326 &            & 16.5 & S    & CSS 1289 \\
85* & 22 08 33.64 & +63 34 54.0 &G& 4267-2710 &            & 15.2 & C    & V513 Cep \\
86  & 22 09 47.53 & +61 09 36.2 &G& 4263-1284 & 22081+6054 & 14.8 & MS   &  \\
87  & 22 23 54.88 & +57 00 16.5 &A&           & 22220+5645 & 16.3 & S    & CSS 1297 \\
88* & 23 14 52.69 & +49 37 40.9 &T& 3631-1405 & 23125+4921 & 12.8 & S4,3 & BD+48\deg3979 \\
89* & 23 37 39.74 & +58 50 45.9 &g&           & 23352+5834 &      & S    & V850 Cas \\
90  & 23 46 18.48 & +66 49 27.6 &G& 4293-0030 & 23439+6632 & 16.5 & MS   &  \\
91* & 23 57 21.31 & +58 25 03.7 &A&           & 23548+5808 & 16.6 & S:C: & V653 Cas \\
\hline
\end{tabular}
\end{center}

\small

Notes:

\begin{tabular}{rl}
 1 &  the proper-motion star G 217-32; position is for epoch 2000; probably not S type \\
 6 &  Dolidze position grossly in error \\
 7 &  BD +21\deg255 = DO 8975 (K5) \\
11 &  middle star in a 20\arcs~arc of three \\
12 &  CSS 55 = MSX5C G132.8280+02.7717 \\
14 &  MSX5C G135.0340$-$02.3791 \\
16 &  MSX5C G135.1851+01.6128 \\
18 &  [ABC90] maa 28 = MSX5C G136.4983+00.4551 \\
21 &  S1* 52; M star, not S; see CSS rejected stars \\
22 &  MSX5C G137.3620+02.4544; previously erroneously identified as IRAS 02545+6133\\
   &  (wrong Dolidze position, IRAS fluxes are for a nebula) \\
23 &  DO 26880 (N) = MSX5C G141.0116+00.7197 \\
24 &  S1* 55 = CSS 71 \\
25 &  DO 27408 (M2) \\
26 &  CGCS 696 \\
27 &  ID assumes Dolidze chart has wrong star marked \\
28 &  Dolidze position switched with star 30, {\it cf.} \\
29 &  NIKC 5-7 = MSX5C G170.6337$-$03.7048 \\
30 &  Dolidze position switched with star 28, {\it cf.}; in open cluster NGC 1798 \\
32 &  MSX5C G174.3450$-$01.4985 \\
33 &  MSX5C G173.7492$-$00.3139 \\
34 &  MSX5C G179.0448$-$03.5796 \\
38 &  MSX5C G179.7805$-$01.7574, IRAS position poor \\
40 &  not confirmed as S type by Stephenson (1984), but 2MASS $J-K = 1.6$ \\
41 &  MSX5C G180.6024+01.5613 \\
46 &  previously erroneously identified as HD 252257 (F5) = BD +31\deg1209, for which \\
   &  Tycho-2 $B-V = 0.54$ \\
\end{tabular}

\newpage

\begin{tabular}{rl}
47 &  MSX5C G187.4163+02.0648 \\
49 &  MSX5C G190.4408+02.7191 \\
52 &  MSX5C G209.2346$-$01.5810 \\
54 &  MSX5C G205.8757+01.7297 \\
55 &  CSS 251 \\
56 &  also CSS 253:  CSS has $-$30\arcm~Dec typo; MSX5C G206.2205+01.7840 \\
61 &  CGCS 1610 = CSS 323; Dolidze $-$1\mm/+10\arcm~position error.  CGCS 1610 previously \\
   &  erroneously identified as GSC 5406-1554, for which Tycho-2 $B-V = 0.43$ \\
62 &  same as CGCS 1687 \\
63 &  late-M type according to Stephenson CGCS reject list \\
65 &  MSX5C G014.6028$-$01.7665 \\
68 &  DO 18567 (M6) \\
69 &  CGCS 4693 \\
72 &  DO 19014 (M5); S4,6 (Stephenson 1984) \\
73 &  Kiso C3-26 \\
75 &  MSX5C G077.9334$-$04.0741; previously erroneously identified as IRAS 20438+3622,\\
   &  which is another red star in the field \\
76 &  CSS 1240 \\
77 &  Dolidze notes that CH and BaII are possibly present in the spectrum \\
78 &  MSX5C G081.0885$-$02.7369 \\
79 &  CSS 1256 \\
80 &  ID assumes Dolidze chart has wrong star marked \\
81 &  MSX5C G092.7896$-$03.1822 \\
82 &  MSX5C G095.6156$-$01.7247 \\
83 &  this star is {\it not}~IRAS 21540+6341 = V500 Cep, which is a much fainter star 3\arcm~north \\
   &  in the open cluster Berkeley 93 (and probably an M-supergiant, not a carbon star) \\
84 &  MSX5C G103.3386+03.5334 \\
85 &  CGCS 5591; the carbon star was previously erroneously identified as GSC 4267-1485, \\
   &  which is a blue star (Tycho-2 $B-V = 0.23$) \\
88 &  CSS 1326 = DO 42750 (M4);  Dolidze $-$1\hr~RA error \\
89 &  type M5/7 in Dolidze (1975b) \\
91 &  CSS 1344 \\
\end{tabular}

\large

\references

Dolidze, M. V., 1975a, {\it Byull.\ Abastumanskaya Astrofiz.\ Obs.}, {\bf 47}, 3 %\BIBCODE {1975AbaOB..47....3D}

Dolidze, M. V., 1975b, {\it Byull.\ Abastumanskaya Astrofiz.\ Obs.}, {\bf 47}, 171  %\BIBCODE {1975AbaOB..47..171D}

Gray, W., 1999, {\tt http://www.projectpluto.com/gsc\_act.htm}

H{\o}g, E., Fabricius, C., Makarov, V. V., Bastian, U., Schwekendiek, P., Wicenec, A., Urban, S. E., Corbin, T., and Wycoff, G., 2000, {\it Astron.\ Astrophys.}, {\bf 357}, 367   % \BIBCODE {2000A&A...357..367H}

Lortet, M.-C., Borde, S., and Ochsenbein, F., 1994, {\it Astron.\ Astrophys. Suppl.\ Ser.}, {\bf 107}, 193 ; see also {\tt http://vizier.u-strasbg.fr/cgi-bin/Dic-Simbad}   % \BIBCODE {1994A&AS..107..193L}

Monet, D., Bird, A., Canzian, B., Harris, H., Reid, N., Rhodes, A., Sell, S.,
Ables,~H., Dahn, C., Guetter, H., Henden, A., Leggett, S., Levison, H.,
Luginbuhl, C., Martini, J., Monet, A., Pier, J., Riepe, B., Stone, R.,
Vrba, F., Walker, R., 1998, USNO-A2.0; U.S. Naval Observatory, Washington DC;
see also {\tt http://www.nofs.navy.mil}

Price, S. D., Egan, M. P., Carey, S. J., Mizuno, D. R., and Kuchar, T. A.,
2001, {\it Astron.\ J.}, {\bf 121}, 2819   % \BIBCODE {2001AJ....121.2819P}

Skiff, B. A., 1997, {\it IBVS}, No.\ 4417  % \BIBCODE {1997IBVS.4417....1S}

Skrutskie, M. F., 2000, {\tt http://www.ipac.caltech.edu/2mass}

Stephenson, C. B., 1984, {\it Publ.\ Warner \& Swasey Obs.}, {\bf 3}, 1  %\BIBCODE {1984PW&SO...3....1S}

Stephenson, C. B., 1989, {\it Publ.\ Warner \& Swasey Obs.}, {\bf 3}, 53  %\BIBCODE {1989PW&SO...3...53S}

Stephenson, C. B., 1992, {\it Astron.\ J.}, {\bf 103}, 263
% \BIBCODE {1992AJ....103..263S}

STScI, 2001, {\tt http://www-gsss.stsci.edu/support/data\_access.htm}

Zacharias, N., Urban, S. E., Zacharias, M. I., Hall, D. M., Wycoff, G. L.,
Rafferty, T. J., Germain, M. E., Holdenreid, E. R., Pohlman, J. W.,
Gauss, F. S., Monet, D. G., and Winter, L., 2000, {\it Astron.\ J.}, {\bf 120},
2131  % \BIBCODE {2000AJ....120.2131Z}

\endreferences

\end{document}
