1 Triple star with 5" distant companions, the brighter being mag. 11.5 pg, spectrum F2 (VB). 2 All bands weak. 7 Nearly pure S. 9 HD catalog: Like Pi 1 Gruis. 12 HD catalog: Like R And. 18 Extremely strong D line. 25 A rare bird. 28 HD catalog: Like R And. See also K66. 36 Very strong sodium D lines. 44 A carbon star is a few arc minutes away. 45 D 8975(K5), Ste(M2S). 65 All bands weak. 67 No TiO, on the 4 degree red plate. 73 All bands weak. 81 Such a spectrum would appear merely M on the infrared plate used by Nass54. 84 Two plates. 90 The position is an estimate by me from a Case infrared objective prism plate. The star is probably one observed by 90 Bidelman in trying for SX Cam, and K gives the type for SX Cam itself from Bidelman's plate. SX Cam is a late M 90 (Bid65, Ste). The present star, on the infrared plate mentioned, is M2 without visible LaO, but this is consistent 90 with the K classification. 92 NassCam thought the absorption in the 7900 A LaO region unusually broad. 97 Two plates. 99 K quotes Blanco that the spectrum may show infrared CN on on objective prism plate. 103 Also Ste. HD catalog: resembles class R. 105 Nass54(M2r). 108 D 28597(M2). 111 Nass54 1-39(Mr), Sharp(M0 III) 114 +14:777, 4o 1 Ori. 116 S-WS 34, Ste. 117 This star, with others somewhat like it, was first discussed by Bidelman (1950, 1954b). See the text references on 117 C-S stars. 118 D 28924(M1). 1.2' from No. 119. 119 1.2' in 145d from No. 118. Underexposed, but the ZrO is definite. An infrared Schmidt plate shows like an M2 119 star. A, but not B, is in the Astrographic catalog and the AGK3. 120 Not the nearby DK Aur, which is a carbon star. On a poor red plate, I find a faint early M near Dolidze's MS star 120 position. 123 All bands weak. 129 Two plates. 131 34738(Ma), -22:1070, BidMac(S), Ste(S). 133 -8:1099. HD catalog: like Pi 1 Gruis. 140 Close to a confirmed carbon star. 148 Dol62a's position differs 10' from the Case one (cited here). 149 BlancN(Mr). +31:1050, B3(III) according to Bouigue et al, Haute Prov. Publ., Vol. 5 No. 49, is only about 2' away. 149 BlancN used infrared plates, which would have shown the star only as M. 151 About 2 s west of B.D. +10:842. 158 D 1262(M2). 159 M8 by Vogt, Astron. J. 78, 389. 165 Dol62a 10(S), Bidun(S), Ste(S), Nass54(M0r). 178 -38:2333. 181 D 11852(M3). 191 On my red plate the TiO type is not even as late as M4. 212 44544(Pec), +3:1214, MSB 19(S), S-WS 48(S:), NassSte(Sp), BidMac(S). One of the better known C-S stars. 219 Ste(S or MS) 222 TiO weak to absent. 225 TiO weak. 230 -43:2537. 231 The infrared magnitude is from Hetzler (1937), who quotes V-I = 4.6. 243 12.5 s west, and 1'39" north, of the C-S star V372 Mon. 244 -4:1617, Ste65(C-S). On an infrared objective prism plate it was noted as similar to W Cas by Nassau, Blanco, and 244 Morgan (1954); that is, they suspected both weak CN, like a weak carbon star, and LaO, like an S star. I did not 244 certainly confirm LaO on an infrared-region slit spectrogram (cf. Astrophys. J. 150, 543, 1967) but there is abundant 244 CN both in the infrared and red. The star is further discussed by Greene (1971). 246 GR Aur has a published position 4' from this one. The published chart is inadequate for my material. 247 +25:1397. 251 Dol62a 11 appears as catalog no. 173 in the first edition because it was originally published with plus declination. 251 The error is corrected in Abast. Bull. 47, 10. 260 +5:1414, BidMac. 263 MacCon: ZrO is weak. 265 -20:1589. 266 A pure S, without TiO. 272 TiO and ZrO are both strong. 277 NassCam(M2), Dol62a 12. The original error in decl. for Dol62a 12 is corrected in Abast. Bull. 47, 10, but the star 277 was already tentatively included with the other designations in the first edition of the S-star catalog. 279 Hetzler VII-14. Hetzler gives V-I = 6.1. 283 +55:1154, Ste(M6,S!e). See also WPB. 297 Found in our southern Luminous Stars survey, but omitted from the first ed. of the S star catalog for being too weak. 300 C.P.D. -19:1672; not in the S.D. 307 +22:1577, Ste(S!). HD catalog: Spectrum resembles class R. 309 About 5 s east of +0:1805. 312 +69:413. 316 Bid65: Strong TiO. 323 Ste(S), BidMac(S), Nass54(M1r). 329 MacCon also noted that ZrO was somewhat weak. 336 About 5' from the listed position of CSV 100853. 341 Perr61. The GCVS does not identify with the B.D.; Perr61 does so as well as with the variable. 344 -8:1900, Ste(S), BidMac(S). This star has the strongest known ZrO among all that I have called C-S. See also Greene 344 (1971). 346 Also Ste. Evidently has strong infrared CN, as it has been classified a carbon star from that region; see Table 2 346 (rejected carbon stars) of my carbon star catalog. It looks type S on a red Case objective prism plate. Dean is 346 cited for the spectral type because he used a slit spectrogram. 347 +46:1271. 348 The GCVS gives the magnitude range as 12.4-12.9 p, but one of my objective prism plates gives the calibrated estimate 348 14.5p. 350 58881(Rp), -11:1941, Ste. HD catalog: like Pi 1 Gruis. 362 Not the nearby no. 791 in the first edition of my carbon star catalog. 370 Near, but different from, the large proper motion star BD -31:4761. 371 Henun 26, West'd. 374 HP Pup, a well-studied RR Lyrae star, has coordinates only about 1' different from these. 378 -15:1953. 382 +14:1729, HR 2967, D 13345(M5). 387 -10:2171. HD catalog mentions that the violet spectral region is weak, and likens the red region to class Mc. To- 387 lolo material shows the star is quite red and that the D lines are quite strong. 390 62340(Pec), -70:463, Henun 28. HD catalog: probably class R. 392 About 1' north of B.D. -10:2177. 401 The SteTerr lpv classification was based purely upon the spectrum, but a comparison of MacCon's 10-degree red plate 401 with my 4-degree red one clearly shows that the star is strongly variable in visual mag.; it is >2 mags. fainter on 401 my plate with the H-alpha emission (and no visible ZrO) than on MacCon's, where it is brighter in the red region than 401 the nearby B.D. star -22 d2296, with which MacCon confused it. 403 +24:1778. HD catalog: spectrum probably resembles R And. 407 Wray 27(Sp), Henun 30. Blanco and Munch noted strong LaO. 411 -18:2040. HD catalog notes the spectrum is similar to Pi 1 Gru in the 4700 A region. 412 Strong TiO. 414 The red-region TiO is stronger than anticipated from the appearance of the blue region. 418 A slit spectrogram confirms the ZrO. 422 -11:2141. Also BidMac. HD catalog: Spectrum somewhat like that of Pi 1 Gru. 424 TiO and ZrO are both strong. 426 Not DF Pup, which is only 2' to the north. 431 H-beta emission noted on a plate covering the 4800-6800 A region. 434 -60:1901, Henun 31. 438 -29:5241. 440 The GCVS lists the maximum as 15p, but one Tololo plate gives 14.2p. The position given here differs about 1' from 440 the GCVS and is based on only one Tololo plate. 442 Independently picked up by me, on a red survey plate, merely as a late M. 454 Well shown, and independently found, on two red Schmidt plates. An undoubtedly variable carbon star (No. 1016 in the 454 first ed. of the carbon star catalog) is nearby, but I have not found it. 455 Not the nearby no. 457. Originally no. 1025 of my carbon star catalog (first ed.), on the basis of an objective 455 prism classification by Rybski. 457 Not the nearby no. 455. The spectral peculiarity on my red-region objective prism plate consists of additional 457 structure in the 6500-8500 A region, like emission lines or (more probably) gaps between strong absorptions. 457 A 10 degree red-region plate of MacCon's confirms the ZrO without showing the 4 degree peculiarities. 466 The carbon classification is by Rybski (unpublished Ph.D thesis, Northwestern University) and on that basis the star 466 is no. 1057 in by carbon star catalog, first ed. A Tololo red plate shows the spectrum only weakly. It is very red, 466 and ZrO does seem to be present. Rybski reported seeing bands of CN but not C2 , but did see H alpha emission. 476 Henun 42, West'd. 487 -26:5801. 489 -29:5912 494 +17:1825. HD catalog: spectrum may resemble that of R And. 506 -35:4598. 524 -17:2543. 526 Sndlk(S), Henun 49(S). 540 Sndlk notes strong D lines. 541 Sndlk(S or MS). 542 BidMac, Henun 53. 543 -32:5649, Ste(S!r), Henun 54. 546 Wray 104. 550 Sndlk(S), Henun 55(S). 556 Hen60(S:). Strong D lines first noted by Henun. 558 Henun 56. 559 No. 1321 in my carbon star catalog, first ed. Case plates (red and blue) show in this position a star which is cer- 559 tainly not carbon, but rather M or weak MS. 562 A computer overlay plus an objective prism plate shows that this is no. 1328 of the carbon star catalog 1st ed., and 562 is S. 589 +31:1946. 591 Sto IV-13, Henun 64. 614 Henun 68. BM note very strong infrared LaO. Ste noted strong D lines, and Henun moderately strong D lines. 617 Ste(S!), BidMac, Henun 69. 619 A Westerlund carbon star, for which he gives V = 16.0, I = 11.2, is within 3' of this position; I of course do not 619 see it. 625 -46:5417. 628 No. 1533 in my catalog of carbon stars, first ed. A blue and red Tololo plate show the star is clearly not carbon, 628 but perhaps weak S. 629 Wray 158(C). Ste: blue spectrum resembles that of R CMi. This star was already excluded from my carbon star cata- 629 log, see Table 2 (rejects) of that publication. 652 Wray 178. 656 A deep ten-degree red objective prism plate lent me by D. J. MacConnell shows that the nearby bright Wray carbon star 656 noted in the first ed. of the carbon star catalog is spurious. 661 Henun 84(Se:). 664 -60:2927. Henun notes strong D lines. 669 This is no. 1647 in the carbon star catalog, 1st ed. 674 Strong D lines first noted by Hen60. Published in Ste73 as a new C-S star, but earlier so noted by CatchF. 676 Sndlk notes strong D lines. 677 Probably identical with the Wray carbon star, no. 1671 of the carbon star catalog. Me by BidMac from the blue spec- 677 tral region. I have no plates on this position. 687 Also Sto III-34, whose position we adopt here, supported by a computer overlay plus a MacCon 10 deg red plate. 692 Henun 94. 693 No. 1722 in the carbon star catalog, 1st ed. A Tololo blue plate shows that the star is clearly not carbon, but M. 693 The fact that I do not see the blue-region ZrO at 600 A/mm is not at all inconsistent with Henun's higher-dispersion 693 classification from the red spectral region. 695 Henun 96. 696 -51:4956. 699 Henun 98. 702 Also Ste. 704 Henun 101. 710 Henun 103. BM note that the infrared LaO is weak. Their published right ascension is in error by 1 m. 714 -52:4068. 719 Henun 107, West'd. 720 -55:3814. 724 Henun 109. The Tololo Balmer line emission decrement indicates that this star is a long-period variable. The CSV 724 quotes mags. 14.1-16.8p, but this is merely from the Bruce Proper motion survey; 12.4p is observed on a Tololo plate, 724 on which the blue-region ZrO is quite weak. The red-region ZrO on the Tololo plate is quite strong, as opposed to 724 the previous sentence and to Henun's classification; obviously the spectrum varies appreciably, in keeping with being 724 a Mira-type variable. 726 1.7' from 1st ed. carbon-star catalog no. 1816, which is also one of W's stars. My red Schmidt plate shows an early 726 M of about the right mag., with a hint of ZrO. W's V mag. for the carbon star puts it near my plate limit. 728 Henun 111, West'd. 729 Houk: M2II-III. 742 Henun 114, West'd. 757 The quoted position is a measurement of only one Tololo plate, but confirmed by computer overlay. It is about 4' 757 south of Wray's position, but is the only candidate in the area on the Tololo plate. 766 Not the nearby carbon catalog no. 1917 (1st ed.). 778 -55:4354, Henun 119. 780 An odd one. ZrO strong and narrow. 787 See also Astrophys. J. 186, 589. 788 Strong D lines first noted by Henun. 794 Wray 250, Henun 122. 795 -47:7642. 796 Houk: M2II/III. 799 Tololo plates underexpose this star, but suggest hydrogen emission. Both facts, coupled with Wray's being able to 799 classify the spectrum, support the CSV identification. 800 The Balmer emission-line decrement indicates a long-period variable. The quoted position is a mean of two accordant 800 plates. 801 -25:9367. 803 +61:1313, Ste(Se). HD catalog: spectrum resembles that of R And. 804 110994(Ma), -89:10. 809 No star is in this position, unless at the plate limit, on a red-region Tololo plate. Either the star is variable, 809 or it is a mis-position for the nearby Wray 256. 811 Henun 131. An unusual case, in that the S character of the spectrum on Tololo plates is more apparent in the blue 811 spectral region than in the red. Variability is thus suggested, although the Wray and Ste magnitude estimates are 811 identical. 814 114586(Np), -56:4829, Henun 133(S5,4). HD catalog: "Spectrum combines features of class M and N." This is merely a 814 primitive description. P. S. The has kindly sent me a print of the objective prism spectrum in the blue. 816 115236(K5p), -44:8539, BidMac(Sp), Henun 135(S:), CatchF(SC). The strong depression of the violet spectral region, 816 that characterizes all the SC and CS stars, was for this star first mentioned in the HD catalog. Strong D lines were 816 first noted by Henun. UY Cen is one of several stars commonly cited as prototypes of the C-S class. The quoted 816 position is from the GC. 817 This star may have exhibited bands of both ZrO and C2 , separately at different phases; see Astrophys. J. 186, 817 589. 819 +44:2267, Ste. 820 Henun 136, West'd. 826 -71:963. 829 A red-region slit spectrogram confirms that this is a weak but definite S star. 830 -52:5798, BidMac(Sp). 831 My confirmation of this star as S-type is based on a red objective prism plate lent me by D. J. MacConnell. 832 -54:5405. 834 120460(Md), -59:4943. The HD catalog reports that H delta is bright on one plate. 837 Ste(S!), Henun 142. The quoted right ascension is the average of Wray and Ste, and the quoted declination is from 837 the GCVS. The Ste declination is -66:47'39" -- in agreement with the GCVS -- but Wray's is more than 2' further 837 south. 838 Near, but different from, the weak carbon (C-S) star no. 2138 of my carbon star catalog, 1st ed. 839 -41:8409. 841 Near a MacCon carbon star. 842 Henun 144. 845 This is a Wray carbon star, no. 2151 of the carbon star catalog, 1st ed. A Tololo red objective prism plate plus a 845 computer overlay shows only one candidate star, overexposed. 846 Not the nearby V635 Cen. 847 Too faint for me to verify that this is a different star from no. 2159 of the carbon star catalog 1st ed. 850 Wray 277(C), Ste(Sp), Henun 146. Hydrogen emission detected by Ste. On a blue-region Tololo plate there is a curi- 850 ous broad depression between 4226 A and Ca H and K which is not CN. Wray 277 also occurs in Table 2 (rejected carbon 850 stars) of my carbon star catalog. The published position (Wray 1966) of Wray 277 is 5.4 s E and 36" S of Wray 850 276 (the S star); Tololo plates show only one star. The position given here is the Tololo position, based on three 850 plates. 853 Houk: M2 III. 856 +84:323. HD catalog: spectrum resembles that of R And. Hetzler (1937) gives V-I = +3.5. 861 Ste(M0e), Henun 148(S), West'd(S). H alpha and H beta emission, but no definite ZrO, seen on my Tololo plates. 864 -37:9747. 867 -60:5373. 870 Also West'd. Although evidently variable -- besides Wray seeing H alpha emission, I do not find the star at all on 870 Tololo plates -- it is definitely not the nearby Y Lupi. 872 BidMac(Se), Henun 153. 876 The Papadopoulos and Palomar charts show only one star in this position. I have no spectral plates. 889 -32:10773, CSV 2325. 895 This is a Wray carbon star, no. 2261 of the carbon star catalog 1st ed. , = Wray 287. I have no Tololo plate. 895 Rejected from the carbon star catalog on the basis of MacCon. 899 A Tololo 10-degree plate confirms the S star (MacCon, Ste). The position given here is a slight modification of 899 Henun's, based on a computer overlay. Probably CSV 2446. 903 +48:2334, Ste(M7). 904 -74:1067, Henun 157(S:). Strong D lines first noted by Henize. 906 Marked in the southern Luminous Stars survey, but omitted from the first edition because too dubious. 909 Henun 158. CSV 2541 has this published position, within its 1'-2' uncertainty; there is no identification chart. The 909 suspected variation is 16-17p; Wray and Ste both observe vis. mag. 12.4, but the H alpha emission is of course highly 909 suggestive. 921 Originally omitted by me as too dubious. 923 Henun 161. 926 A slit spectrogram of the red region shows weak but definite ZrO. 931 149511(R5), -30:13283, Ste(S!r), Wray 297(C), Henun 165(S5,8), Sanf41(S). Sto published the spectral type as R, but 931 on query by me found this was an error. Tololo plates show Ca I 4226 quite wide and strong. Already excluded from 931 my first carbon star catalog. 934 A W carbon star, confirmed by Sndlk and me, is about 3' NE of this position, and an M star, probably too bright to be 934 W's S star, is very near his S star position, on a red Schmidt plate. 935 Outstandingly strong D lines noted by Henun and by Ste. 936 Henun 167. The CSV quotes the declination 1' different from the discoverer's, whose identification chart field I 936 could not locate on the Wurzburg Atlas even after finding the S star on the latter. 940 Henun 168(S4,6; strong D lines). The GCVS notes that the star lies in a nebula. 943 As a Rybski carbon star this is no. 2371 in the 1st ed. of my carbon star catalog, and as a Henun S: it should have 943 been, but was not, included in Table 2 of my first S-star catalog. 947 Henun 170. 948 No. 2381 in my carbon star catalog, 1st ed., on the basis of Wray's classification. A red Tololo plate shows a late 948 M star with probable weak ZrO. 950 Contained in my carbon star catalog table of rejected stars because MS, but omitted from the first ed. S-star catalog 950 because too weak. 954 153858(Mb-Md). 964 +5:3352. A Case red-region objective prism plate shows M2-3 without ZrO, but is too overexposed to show weak ZrO. An 964 M4 star, less than a magnitude fainter, is 3' to the northeast. 967 MacCon's published position is that of a nearby bright A-type star. 969 A Wray carbon star, hence no. 2426 in the 1st ed. of my carbon star catalog. 974 -41:11533, Ste, Henun 175. The HD catalog likens the spectrum to those of Pi 1 Gru and T Cam. 976 -14:4618, Nass64 4-1, Henun 207. Strong D lines on a Schmidt plate. For some early problems with nomenclature for 976 this star, see the first edition. 978 157335(Ma), FT Ser, -28:13088, Henun 178. Strong TiO. 994 -53:7361, Wray 314(C). The HD classification supports Henun's spectral type rather than Wray's. No. 2468 in my car- 994 bon star catalog 1st ed., on the basis of Wray's classification; but the HD type was already pointed out in the car- 994 bon catalog. 997 Also NassSte. 999 20" from a brighter M1 star. 1000 A Wray carbon star, no. 2485 in the 1st ed. of my carbon star catalog. A Tololo Schmidt plate plus computer overlay 1000 confirms MacCon; it is a clearcut S. 1004 320767(Me), Henun 181. 1010 -30:15065, Sndlk(MS:), Henun 182. 1013 Strong TiO. 1014 -65:2417. 1016 Henun 209. 1018 A Tololo red plate, which should be deep enough, shows no candidate star within a 4'x4' square centered on this posi- 1018 tion. A Westerlund carbon star, V mag. 13.5, has a published position some 3' from this one and also does not show, 1018 but the plate may not go that faint. 1020 Henun 184. 1021 Omitted from the first edition of this catalog because I could find no candidate star by offsetting from Henun 184 1021 (no. 1020 of the present catalog). 1023 -36:12264. 1025 -67:2205. 1026 Sto(N), Henun 188, Ste(S). No. 2543 in my carbon star catalog, 1st ed., on the basis of the Sto classification. Blue 1026 and red Tololo plates confirm that this is an S star. 1043 Henun 210, V385 Sct. 1044 No. 2581 in my carbon star catalog 1st ed., on the basis of the Wray classification. A Tololo red plate clearly 1044 shows that the star is a good S-type. 1052 Nass54(M3r). It is normal for such stars to appear as M or reddened M on plates of the sort used by Nass54. 1053 +36:3157. 1054 Sndlk, Henun 212. 1056 -35:12728. 1058 Strong D lines (Sndlk). 1070 172804(Np), NassCam, NassSte. HD catalog: Spectrum may resemble that of T Cam. 1071 CSV 7917. Originally announced by Apriamishvili as a nova, but it is some other type of variable. See the remarks 1071 in the first edition of the S-star catalog, plus Var. Star Bull. 966, for more details. 1083 WPB mentions Bidelman having observed strong SrI 4607 and that all oxide bands are weak. 1084 Two plates. 1091 Houk: M2/3. 1092 +23:3516. 1093 A now well known C-S (or SC) star originally discovered by me as "Case 621". Also listed in the carbon star catalog. 1099 +12:3780. Near, but different from, S-WS 14 (no. 1101 this catalog). 1100 See note for no. 1100. 1104 The discoverer announced this star as variable, and on that basis it is no. 11755 in the 1982 edition of the CSV. 1112 Henun 216(Se). Strong D lines first reported by Henun. The infrared CN is at times as strong as in many carbon 1112 stars (Terrill, Astron. J. 74, 413, 1968). 1115 Spectrum at minimum composite according to Herbig, Astron. J. 71, 779, 1966. 1117 -17:5546, Ste(S!). HD catalog: class Se. The GCVS notes an F-type companion within 1"; see also the Herbig refe- 1117 rence for no. 1116. KB: At the 1966 maximum, Palomar Coude spectrograms by Greenstein and Keenan showed the strongest 1117 Li 6707 line yet observed in an S star. 1118 D 5515(M0). 1123 Balmer emission reported by Catchpole & Feast, Observatory 91, 29, 1971. 1130 The position in MacCon82 differs almost 1' from ours (given here). A computer overlay supports our position. 1135 CSV 4665. 1137 MacRae says variable. 1138 Strong TiO, like M5-6. 1141 Vys 19(S4), NassCam, NassSte, Henun 217(S7,7). EP Vul, then nameless, was first recognized as a red star (V-I = 8.0) 1141 by Hetzler (1937), and as an S star by Rust (1938). The star has often been referred to as CE Vul, apparently first 1141 by K; but the identification chart for EP Vul (which is at pains to show also the nearby CE Vul) plus Case and Ham- 1141 burg objective prism plates make it clear that the only S star in the region is EP Vul. I cannot certainly locate CE 1141 Vul on any of these plates, which are blue, red, and infrared. The Cal Tech infrared survey (Neugebauer and Leighton 1141 1969) quotes a position in excellent agreement with the accurate NassSte one (the latter based on two plates). Schai- 1141 fers (Mitt. Verand. Sterne, No. 385, 1959), looking for EP Vul because it had no published spectral type, evidently 1141 found it, and misclassified it as a carbon star; and Table 2 (rejected carbon stars) of my 1st ed. carbon star cata- 1141 log corrects this to S, although I was not then aware that EP Vul was already published as an S star in the guise of 1141 CE Vul. Schaifers' classification was done from the infrared, hence the CN bands must at times be strong, although 1141 I have not seen this. 1145 Hetzler IV-1. Hetzler (1937) gives V-I = 8.5 mag. The Hetzler-S-WS identification given here is based on Hetzler's 1145 published chart. 1149 The NassSte classification is based on a red-region objective prism plate; they note that an infrared objective prism 1149 plate gives the type M6. In the blue region, one 600 A/mm Hamburg plate shows a washed-out (overlapped?) M or S 1149 spectrum. 1150 +49:3064, Merr(Se), Ste(S!e). 1152 The position given here, from one of my survey plates, differs by several arc minutes from some previous publica- 1152 tions, but has been checked by computer overlay. 1159 Nass64 deduced that this is a long-period variable from the hydrogen emission decrement. They also observed a magni- 1159 tude of 12.9p, somewhat brighter than the maximum given by the GCVS. 1161 Henun 218. 1164 The spectral type in WPB is by Sanford, unpublished. An infrared objective prism plate shows extremely strong LaO. 1165 +32:3593, Merr(MS), Henun 220(S:). 1168 A red-region slit spectrogram confirms that the star is weak S. 1170 Houk: M1 III. 1177 The GCVS spectral type is evidently from Nassau and Van Albada, Astrophys. J. 107, 418, 1948, which gives a chart but 1177 no position. 1180 Also Ste(S!e). 1185 The only plate of mine that shows this star is a 1700 A/mm infrared objective prism plate. On it, the star looks 1185 very red, without absorption bands. 1188 +36:3852, Merr(MS), NassSte(S), Henun 221(S5,6). The ZrO strength is quite variable. The HD was unsure whether the 1188 underexposed spectrum belonged to class N or S. 1189 D 18567(M6), Henun 222. 1194 Bidelman's observation was of the blue spectral region. I have obtained a red-region slit spectrogram that shows the 1194 6474 ZrO quite strongly. 1195 Bidun, Henun 197. 1196 -44:13831, Henun 198. HD catalog: Spectrum is similar to class N, but does not belong to that class. 1198 192446(Mb), +16:4199. 1200 +76:784, Merr(Se), Ste(Sr). The HD catalog noted that the spectrum might be of type S. K quotes Blanco that the in- 1200 frared LaO is strong. 1203 The position given here is from one of my survey plates, and differs 3' from the GCVS one which was given to only 1'. 1203 The published blue-magnitude identification chart has too small a field to be useful with my red-magnitude plate. The 1203 variable discoverer did say that the star was red. 1208 Henun 225. 1211 +0:4492, Ste(M8). The star was picked up in my survey merely for being late M. The weak ZrO is not visible on my 1211 survey plate. 1217 Two plates. 1219 Henun 227, Dol65(S), Nass54(M4r), Sharp(S:). 1220 All bands are very weak. There may be no TiO. 1221 All bands very weak; there may be no TiO. 1224 +32:3850, Merr(S), NassCam(S:), NassSte(S), Henun 228(S5,8). HD catalog: spectrum resembles that of AA Cyg. 1225 Two plates. 1226 +16:4290, Merr(MS), Henun 229(S5,4e), Ste(S[e:]). The HD catalog is uncertain as to spectral type. 1232 Henun 231(S6,8e). 1235 +8:4506. This star occurred in my 1st ed. carbon star catalog, table of rejected carbon stars, where I say it is 1235 type S, but was inadvertently omitted from my previous S-star catalog. 1253 +28:3944, Vys 13(S4), Henun 234(S6,8), Ste(S!). 1254 D 39057(M6). 1256 There is some evidence of H beta and H gamma emission. 1266 Dolidze's position is 3' further north, still nearer to Tau Cygni. As it is, Tau Cyg makes my available spectral 1266 plates useless for checking the S star. The GCVS star is quoted as very red. 1273 Kurtanidze, unpublished, cites a carbon star 3' south of my S star, whose position has been checked by computer over- 1273 lay. I find a featureless red spectrum in his position. The S star is quite red, with TiO weak (like M0) and ZrO 1273 moderate. 1286 Strong D lines noted on a Case objective prism plate, and mentioned in the first edition of this catalog. KB note 1286 strong CaCl bands and that it is very similar to VX Aql in having a very close abundance balance of carbon and oxy- 1286 gen, as also pointed out in Ake's Ph.D. thesis. It is interesting that fairly strong infrared LaO has been seen on 1286 objective prism plates (NassCam, C. Terrill's thesis, Ste). 1292 Also K66. K's spectral type was based on a description by Vyssotsky of a McCormick plate, which appears to represent 1292 the only time that ZrO has been seen in this spectrum. As a rule, only TiO is seen. 1294 -46:14292, Henun 202(S5,8). A companion 2.7" away has spectral type G0 V and equal radial velocity according to 1294 Feast, Monthly Not. Roy. Astron. Soc. 113, 510, 1953. Pi 1 Gru is slightly variable. 1298 Two plates. 1303 -45:14790, Henun 204. 1304 All bands weak. 1310 NassCam(M4), Ste(MS). 1315 +16:4833, HR 8714, Ste(M2S). 1316 Strong TiO. 1322 +7:4981. IDS lists a 10th-mag. companion, 32" in 198d. 1326 Ste: M4[vwkS::]. 1335 Vys 14(S4e). 1337 This occurs as no. 656 in the 1st ed. of the present catalog, with erroneous coordinates and mis-labelled as Dol68 3. 1342 Also Ste. 1345 Also Ste(S!rr). K quotes Blanco that the infrared LaO is strong. Spectrum at minimum composite according to Herbig, 1345 Astron. J. 71, 779, l966. 1345 Astron. J. 71, 779, l966. 1346 -15:6531, Merr(MS), Ste(M7S).