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## (from tabmap V6.0 (2016-08-18)) 2024-05-21T13:50:05 #--------------------------------------------------------------------------- #-- III/10B G5 and later stars in a North Galactic Pole region (Upgren 1962) #-------------------------------------------------------------------------- #---Table: III/10B/./notes.dat Notes from the original paper (142 records) # NGP A6 --- NGP designation # No I1 --- Line number within a note # Text A72 --- Text of remarks --------------------------------------------------------------------------------- |N| NGP |o|Text ------|-|------------------------------------------------------------------------ 25 56|1|Possible emission line at 3770 angstroms. 25 86|1|M star No. 59. 26 58|1|4 Com. 26 127|1|H line appears weak; possible band at 4570 ang. 27 66|1|M star No. 29. 27 125|1|M star No. 57. 27 143|1|M star No. 65. 28 46|1|Absorption lines at 4075 and 4450 ang. are very strong. 28 56|1|M star No. 34. 28 76|1|M star No. 38. 28 78|1|M star No. 41. 29 13|1|M star No. 15. 29 54|1|M star No. 21. 29 70|1|M star No. 32. 29 77|1|M star No. 36. 29 93|1|Gamma Com. 29 156|1|M star No. 70. 30 28|1|M star No. 20. 30 79|1|M star No. 48. 30 119|1|Double star. 31 57|1|Overlap with fainter star. 31 115|1|M star No. 61. 32 28|1|Strong CN. 32 49|1|M star No. 28. 32 70|1|Double star. 32 82|1|Strong CN. 32 91|1|M star No. 51. 32 115|1|Gliese No. 485. 33 1|1|M star No. 7. 33 21|1|Very strong line at 4175 ang. 33 51|1|Strong CN. 33 118|1|M star No. 58. 34 39|1|Double star. 34 55|1|Strong CN. 34 91|1|Gliese No. 474. Gliese gives its spectral class as gG8 and notes 34 91|2|that its parallax is probably too large considering its small proper 34 91|3|motion and high luminosity. 35 57|1|M star No. 27. 35 90|1|Strong CN. 35 103|1|M star No. 55. 35 112|1|Strong CN. 35 115|1|Strong CN. 35 134|1|Double star. 36 4|1|M star No. 6. 36 11|1|M star No. 11. 36 94|1|M star No. 54. 36 154|1|M star No. 72. 36 157|1|M star No. 75. 37 25|1|M star No. 14. 37 27|1|M star No. 16. 37 48|1|Strong CN. 37 160|1|Strong CN. 38 28|1|Groombridge 1830 = LFT 855 = Gliese No. 451. This star is a well 38 28|2|known subdwarf with a very high proper motion. 38 44|1|M star No. 18. 38 89|1|Double star. 38 101|1|M star No. 45. 38 104|1|M star No. 46. 38 143|1|M star No. 60. 38 181|1|M star No. 78. 39 1|1|M star No. 4. 39 42|1|Strong CN. 39 88|1|Strong CN. 39 89|1|6 CVn. 39 134|1|M star No. 67. 39 141|1|Overlap with fainter star. 40 5|1|Strong CN. 40 49|1|Peculiar. H and K lines are weak, 4215-ang. CN band is very strong 40 49|2|and the continuum to the long-wave side of the G band is depressed. 40 49|3|Probably not a composite spectrum. 40 60|1|M star No. 19. 40 82|1|M star No. 24. 40 83|1|M star No. 26. 41 39|1|M star No. 12. 41 74|1|M star No. 22. 41 85|1|2 CVn. Partially overlapping slightly fainter companion of spectral 41 85|2|type F5. 41 93|1|Strong CN. 41 98|1|M star No. 42. 41 127|1|Strong CN. 41 148|1|M star No. 68. 41 165|1|M star No. 76. 42 8|1|M star No. 3. 42 87|1|M star No. 33. 42 99|1|Strong CN. 42 100|1|M star No. 37. 42 115|1|M star No. 49. 42 118|1|M star No. 50. 42 136|1|M star No. 56. 42 148|1|M star No. 63. 43 10|1|G band appears weak. 43 20|1|M star No. 9. 43 62|1|LFT 871. 43 151|1|M star No. 62. 43 186|1|M star No. 74. 44 14|1|M star No. 8. 44 85|1|M star No. 31. 44 120|1|M star No. 52. 44 154|1|Strong CN. 44 155|1|M star No. 73. 44 164|1|M star No. 79. 45 3|1|LFT 832. Partially overlapped by brighter companion, LFT 831. 45 16|1|M star No. 5. 45 33|1|Variable star? 45 42|1|Peculiar. This star appears very similar to HR 7606, which is 45 42|2|discussed by Bidelman (1957, PASP 69, 573). The uv portion of the 45 42|3|spectrum is too strong for a G8 star. This star is probably of 45 42|4|spectral type G0 with abnormally strong CN bands. 45 49|1|M star No. 17. 45 69|1|M star No. 25. 45 100|1|M star No. 40. 45 114|1|M star No. 47. 45 137|1|Strong CN. 45 163|1|This star is probably a "lambda 4150 star" as defined by 45 163|2|Roman (1952, ApJ 116, 122). 45 169|1|M star No. 77. 46 33|1|M star No. 13. 46 56|1|Strong CN. 46 76|1|M star No. 43. 46 85|1|M star No. 53. 46 107|1|M star No. 64. 46 121|1|M star No. 80. 47 23|1|M star No. 2. 47 76|1|Strong CN. 47 92|1|Line at 4175 ang. is abnormally strong, as is the H9 line at 3835 ang. 47 109|1|M star No. 35. 47 124|1|M star No. 44. 47 146|1|Strong CN. 47 156|1|Strong CN. 47 159|1|M star No. 69. 47 161|1|M star No. 71. 48 6|1|Strong CN. 48 21|1|Chi UMa. 48 99|1|Strong CN. 48 114|1|M star No. 66. 49 16|1|M star No. 1. 49 32|1|M star No. 10. 49 71|1|M star No. 30. 49 78|1|3 CVn. 50 65|1|M star No. 23. 50 77|1|M star No. 39. 50 106|1|Strong CN. ---------------------------------------------------------------------------------