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