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## (from tabmap V6.0 (2016-08-18)) 2024-05-05T14:37:16
#---------------------------------------------------------------------------
#-- 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
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|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.
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