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## (from tabmap V6.0 (2016-08-18)) 2024-03-19T07:49:27 #--------------------------------------------------------------------------- #-- III/76A Luminous Stars in the Northern Milky Way (LS) (Hardorp+ 1959-1965) #-------------------------------------------------------------------------- #---Table: III/76A/./notes.dat Remarks originally in volumes II, IV and VI. (167 records) # LS A7 --- *LS number, as in the file ls.dat # Vol I1 --- *[1/6] Volume number, as in the file ls.dat # Text A71 --- Text of note #Note on LS, Vol: # Columns are repeated when the note requires several lines. #------------------------------------------------------------------------------- --------------------------------------------------------------------------------- |V| |o| LS |l|Text -------|-|----------------------------------------------------------------------- +40 1|2|May be B7 II. +39 47|2|May be cA. +39 55|2|ADS 14314AB. The published delta m (Aitken, A New General Catalogue +39 55|2|of Double Stars Within 120 deg of the North Pole) is so large that +39 55|2|the observed spectrum must actually be entirely that of the primary. +39 55|2|The primary is said to be composite in the Henry Draper Catalogue, +39 55|2|and for this reason the star is given two HD numbers, HD 198287/8. +39 55|2|The spectrum does not appear composite on our plates, and was charac- +39 55|2|terized by Hynek (Perkins Contribution 1, No. 10, 1938) as one simu- +39 55|2|lating compositeness because of high luminosity. This conclusion is +39 55|2|almost certainly correct. +38 17|2|May be B6 Ia. +38 83|2|May be B7 Ib. +37 35|2|May be B8 II. +37 72|2|May be B7 Ir. +36 8|2|May be B7 II. +36 11|2|May be cA. +36 86|2|ADS 14724A. +35 33|2|ADS 13374A. +35 61|2|May be B9 II. +35 73|2|May be cA. +34 12|2|May be B8 Ib. +32 15|2|ADS 13335A. +31 1|2|H-beta in emission. +31 15|2|The type given here is purely descriptive; among the grounds for +31 15|2|doubting it is the fact that the spectrum shows no reddening despite +31 15|2|its low Galactic latitude. On the plate covering its position, an +31 15|2|absorption feature which may be H-gamma is strong, while all other +31 15|2|features, including the Balmer discontinuity, are at the limit of +31 15|2|visiblity. +30 17|2|May be B7 II. +30 37|2|HR 8084. +29 2|2|May be cA. +29 5|2|P Cyg type. Strong H-alpha emission. +29 6|2|Similar to AG Peg. +29 22|2|May be cA. +28 2|2|May be cA. +24 26|2|B7 IV(e), Osawa, Ap. J. 130, 159, 1959. +22 2|2|May be B8 Ib. +22 3|2|ADS 12287AB. +22 6|2|BDS 9287A. +21 7|2|May be cA. +17 3|2|ADS 11884A. +16 4|2|Nucleus of planetary nebula No. 220 in Vorontsov-Velyaminov's catalogue +16 4|2|(Gaseous Nebulae and New Stars, p. 563 ff. Moscow-Leningrad: Soviet +16 4|2|Academy of Sciences, 1948). +16 9|2|Perhaps B7 IIle. +15 7|6|Weak ultraviolet. +13 2|2|May be cA. +13 9|6|Abnormal Balmer decrement. +13 10|2|May be B6 Iab. +11 2|2|ADS 12000AB. +11 2|4|Flat continuum. +11 3|6|K-line possibly present. +11 5|2|Only one absorption spectrum is clearly identifiable in this overlap, +11 5|2|and is assumed to belong to Aitken's component A. +11 7|6|Weak ultraviolet. +11 9|6|Ultraviolet also considered weak in this star. +11 12|6|HR 2370, ADS 5153AB. +10 2|4|Flat continuum. +10 8|6|Nebulosity surrounds the star. +09 3|4|May be composite. +09 13|6|Precedes BD+09 1332 by only a few seconds of arc. +09 14|6|ADS 5322AB, also S Mon; the slit classification is presumably for +09 14|6|component A. +09 15|6|ADS 5327AB. +08 2|4|May be A0 I-II. +08 3|6|May be composite. +08 8|6|Probably not a true Wolf-Rayet, since Hiltner (Ap.J. Suppl. 2, No. 24, +08 8|6|1956) refers to this star merely as showing high-excitation emission +08 8|6|superposed on about an O9 spectrum. +08 11|6|K-line present. +08 12|6|Nebulosity surrounds the star. +07 2|4|May be composite. +07 7|6|K-line and perhaps 4026 present. +06 1|6|Appears to be composite. +06 2|6|K-line may be present. +06 2|4|Very flat continuum. +06 5|4|Flat continuum. +06 6|4|G band possibly visible. +05 3|4|Rather flat continuum. +05 6|4|May be composite. +05 13|6|Probably a double star. +05 20|6|H-epsilon somewhat enhanced. +05 21|6|K-line may be present; ultraviolet weak; composite? +05 25|6|May be composite. +04 1|4|Weak or variable K-line? +04 8|6|May be composite. +04 16|6|Helium I lines appear to be visible. +04 35|6|K-line may be present. +03 6|6|May be composite. +03 12|4|May be composite. +02 13|6|The small angular separation of this binary star assures that the pub- +02 13|6|lished spectral type of B0 III:p pertains to the combined light of the +02 13|6|system. +02 14|6|Possibly composite. +02 16|6|K-line may be present. +01 5|4|May be composite. +01 8|4|May be composite. +01 10|4|May be composite. +00 1|6|AGK2 asumes Aitken's position angle for AC is 180 degrees in error and +00 1|6|calls this star component C; this seems true on a blue plate, but our +00 1|6|red (H-alpha) plate supports Aitken. +00 3|4|Flat continuum. +00 5|4|Classified only from H-alpha plates. +00 10|4|May be B8 II. +00 21|4|Flat continuum. -00 5|4|May be B7 II. -00 7|6|May be composite. -00 15|4|K-line visible? -00 20|4|Composite? -01 1|6|ADS 4141AB. -01 16|6|May be B7 III. -01 18|4|May be composite. -02 1|6|ADS 4241ABC; a published spectral type of O9.5 V exists. -02 3|4|K-line may be variable on our plates. -02 6|4|May be B8 II-III. -02 10|6|The published spectral type of B0.5 IV (2) must refer to the combined -02 10|6|light of both components, in view of their small angular separation. -02 14|4|May be composite. -02 28|4|May be B8 II-III. -03 9|4|Roberts 90. -03 13|6|A spectral type of O9 V has been published for what is presumably -03 13|6|component A. -03 19|6|Flat continuum. -04 8|4|May be composite. -04 14|4|Roberts 89. -04 24|6|May be B7 II-III. -04 33|4|Roberts 91. -05 1|6|May be double. -05 12|6|K-line probably present. -05 30|4|Composite? -06 1|6|Nebulosity surrounds this star. -06 7|4|Roberts 88. -06 11|4|K-line present? -06 29|4|K-line present? -07 3|4|Composite? -07 17|4|Composite? -07 18|4|May be B7 II-III. -07 24|4|May be B8 II-III. -07 31|4|Flat continuum. -08 27|4|K-line visible? -08 29|4|K-line visible? -09 7|6|Ultraviolet continuum weak. -09 10|4|May be B7 II. -09 11|4|Lambda 4686 emission? -09 29|4|K-line visible? -10 11|4|ADS 11414A; component B may be A- type. -10 15|4|May be B7 II-III. -10 16|4|May be B7 II. -10 18|4|Composite? -10 24|4|ADS 11670AB. -10 29|4|Flat continuum. -11 14|4|Roberts 85. -11 15|4|Spectral appearance differs considerably between two plates; may be -11 15|4|less luminous than OB-. -11 20|4|Of? -11 33|4|May be B7 II. -12 5|4|The published spectral type is taken form Hiltner, but does not check -12 5|4|with the star's appearance on our plates. -12 56|4|May be composite. -12 59|4|Classified only from an H-alpha plate. -13 16|4|Close pair, both OB stars, originally classified as one star. The -13 16|4|magnitude refers to the combined light. -13 40|4|Roberts 86. -13 71|4|May be composite. -14 56|4|Roberts 87. ---------------------------------------------------------------------------------