LI-LMC 0143  SHV0453582-690242;
LI-LMC 0153  WOH SG066 = RMMP 045 = SHV0454257-684856
LI-LMC 0253  WOH SG097 = RMMP 087
LI-LMC 0383  WOH SG140 = SP 29-33 = RMMP 151
LI-LMC 0425  WOH SG157 = RMMP 183
LI-LMC 0517  SP 35-1 = WOH SG179 = RMMP 215
LI-LMC 0612  SP 37-24 = WOH SG193 = RMMP 239
LI-LMC 0663  SP 37-35 = WOH SG204 = RMMP 256
LI-LMC 0869  SP 47-6 = WOH SG241 = RMMP 308
LI-LMC 0932  WOH SG257
LI-LMC 0976  RMMP 339
LI-LMC 1038  RMMP 358
LI-LMC 1059  SP 46-16 = WOH SG287 = RMMP 364
TRM 052      SP 45-16 = WOH SG299 = RMMP 383
TRM 073      SP 45-18 = WOH SG301 = RMMP 384
LI-LMC 1103  WOH SG306 = RMMP 390
LI-LMC 1107  HV 5854 = SP 45-23 = WOH SG313 = RMMP 401
LI-LMC 1125  SP 46-32 = WOH SG319 = RMMP 408
LI-LMC 1145  SP 47-17 = WOH SG331 = RMMP 432
LI-LMC 1155  WOH SG337 = RMMP 444
LI-LMC 1163  SP 46-39 = WOH SG338 = RMMP 448
LI-LMC 1170  WOH SG343 = RMMP 468 = R 108
LI-LMC 1172  WOH SG341 = RMMP 462
LI-LMC 1190  SP 45-38 = WOH SG349 = RMMP 482
LI-LMC 1212  SP 47-20 = WOH SG358 = RMMP 505
LI-LMC 1223  SP 47-22 = WOH SG369 = RMMP 519
LI-LMC 1234  SP 51-6 = WOH SG371 = RMMP 531
LI-LMC 1238  RMMP 539
LI-LMC 1241  WOH SG375 = RMMP 545
LI-LMC 1281  SP 46-59 = WOH SG388 = RMMP 575
LI-LMC 1294  WOH SG395 = RMMP 589 = GRV0533-6650
LI-LMC 1304  SP 52-18 = WOH SG401 = RMMP 606
LI-LMC 1360  SP 52-29 = WOH SG422 = RMMP 656
LI-LMC 1364  WOH SG421 = RMMP 655
LI-LMC 1366  SP 52-32 ??
LI-LMC 1399  SP 52-35 = WOH SG432 = RMMP 683
LI-LMC 1553  SP 54-34 = WOH SG467 = RMMP 753
LI-LMC 1559  SP 54-40 = WOH SG473 = RMMP 761
WOH G352     also very close to LI-LMC 1125.
LI-SMC 61    PSC00483-7347. Was not selected because it is mentioned as
LI-SMC 61    slightly extended in Schwering & Israel (Cat. <II/181>); note
LI-SMC 61    that Whitelock et al. (1989MNRAS.238..769W) mention that this
LI-SMC 61    object could also be a pre-main-sequence star.
LI-LMC 1341  near a nebulosity.
LI-SMC  233  Galaxy or PN ? (3 reference for each ...)
LI-SMC   48  near LHA 115-S 9 (B1, V=14.0), and RAW 479 (C:, V=16.3)
LI-LMC  197  near the G4Ia supergiant HD 268759 but only very rough
LI-LMC  197   coordinates are available
LI-LMC  203  near SK-69 39a (A3Iab, B=12.5) and HV 12501 (M1.5, V=11.9)
LI-LMC  493  near BMB-BW49=BM 16-24 (C, I=14.0)
LI-LMC  530  near SHV0510004-692755 (M6, I=14.7, P=169)
LI-LMC  568  could be associated with IRAS-PSC 05112-6843
LI-LMC  595  near BM 18-8 and 18-9 (C)
LI-LMC  644  near HV 2378
LI-LMC  696  near BM 20-13 (C)
LI-LMC  730  near BM 21-13 (C)
LI-LMC  825  could be associated with IRAS-PSC 05205-6913
LI-LMC  987  near HD 269507 (K, B=11.5) but only very rough coordinates are
LI-LMC  987  available. Could be associated with IRAS-PSC 05249-6916.
LI-LMC 1028  near BM 23-21 (C)
LI-LMC 1055  near SK-67 109 (V=13.1)
LI-LMC 1082  near SK-66 97 (B=12.5) and SK-66 98 (B=11.9)
LI-LMC 1378  near BM 33-31 (C)
LI-LMC 1657  near BM 37-32 (C)
LI-LMC 1775  near WORC 220 (C)
LI-LMC 1785  AGN candidate in De Grijp et al. (1987A&AS...70...95D)
LI-LMC 1795  a bright R counterpart is found by Zijlstra et al.
LI-LMC 1795  (1996MNRAS.279...32Z)
LI-LMC 1807  IRAS-PSC06011-6636A
LI-SMC 19    near RAW 179 (C, V=16.8)
LI-SMC 72    near RAW 651 (C, V=17.3), RAW 658 (C, V=17.6), and the cepheid
LI-SMC 72    HV 1522 (V=14.6)
LI-SMC 78    in a cluster ? Near RAW 706 (C, V=17.0)
LI-SMC 96    96 and 97 are probably the same IRAS source. Near RAW 822
LI-SMC 96    (C, V=17.6), AzV 148 (B0, V=14.3), and the Cepheid HV 1598 (V=15.9)
LI-SMC 100   near RAW 832 (C, V=17.3)
LI-SMC 106   near RAW 941 (C, V=17), the Cepheid HV 1649 (V=15.5), and the
LI-SMC 106   foreground red variable Z Tuc (B=13)
LI-SMC 112   near the foreground star HV 5627 (F7V, V=9.5)
LI-SMC 133   near the known or suspected KM supergiants SkKM 187, SkKM 190,
LI-SMC 133   HV 11402, and PMMR 100 (M0.5, V=12.8)
LI-SMC 143   near RAW 1258 (C, V=16.9) and RAW 1254 (C, V=17.1)
TRM 137      near HD 268931 (G, B=12.2) and HD 268933 (F, B=12.2) but only
TRM 137      very rough coordinates are available
LI-LMC 1839  AGN candidate in De Grijp et al. (1987A&AS...70...95D)
LI-LMC  478  According to Israel & Koorneef (1991A&A...248..404I), there is
LI-LMC  478  a M giant or supergiant near the IRAS position. However the
LI-LMC  478  association is doubtful
LI-LMC  435  near the cepheid HV 893
LI-LMC  531  near the M supergiant HV 5625 (V=12.6) and the B5Iab supergiant
LI-LMC  531  HD 269101 (V=12.0)
LI-LMC  541  near BMB-BW097 (M6, I=14.0)
LI-LMC  718  near BM 21-10=SP 38-16 (C)
LI-LMC  794  IRAS-PSC 05191-6936. Near the C star SHV0518595-693653
LI-LMC  832  near the M6 star SHV0520342-693911
LI-LMC 1010  near the IRAS extended structure X0525-662
LI-LMC 1094  near the IRAS extended structure X0527-714
LI-LMC 1292  near a nebulosity
LI-LMC 1315  could be associated with IRAS-PSC 05338-6725
LI-LMC 1336  near HD 269762 (B9Ia, V=11.4), HV 2677 (M3/5, V=13.6), and the
LI-LMC 1336  PN SMP 1-78
LI-LMC 1390  near BM 33-37 and BM 33-43 (C)
LI-LMC 1434  could be associated with IRAS-PSC 05375-6949
LI-LMC 1494  could be associated with IRAS-PSC 05399-6906
LI-LMC 1535  near BM 36-7 (C)
LI-SMC 90    could be identified with IRAS 00515-7455;
LI-LMC 147   could be identified with IRAS 04544-6722;
LI-LMC 838   could be identified with IRAS 05209-7101;
LI-LMC 1812  IRAS 06024-6645A.
LI-LMC 1130  Zijlstra et al. (paper II, 1996MNRAS.279...32Z) find a bright
LI-LMC 1130  R counterpart (SP 44-29), and Reid et al. (1990,
LI-LMC 1130  Cat. <J/ApJ/348/98>) find 2 possible optical identifications;
LI-LMC 1130  the infrared colours indicate that the star is not obscured;
LI-LMC 1130  either the star is not associated with the IRAS source
LI-LMC 1130  (Zijlstra et al.), either it is a hot star, or it is embedded
LI-LMC 1130  in a nebula.