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HD 10132


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Chemical composition of evolved stars of high galactic latitude
We have carried out abundance analysis for a sample of high galacticlatitude supergiants in search of evolved stars.We find that HD 27381 has atmospheric parameters and an abundancepatternvery similar to that of the post-AGB star HD 107369.HD 10285 and HD 25291 are moderately metal-poor andshow the influence of mixing that has brought the productsof NeNa cycle to the surface.The high galactic latitude B supergiant HD 137569 shows selectivedepletion of refractory elements normally seen in post-AGB stars.We find that the high velocity B typestar HD 172324 shows moderate deficiency of Fe group elements butthe CNO abundances are verysimilar to that of disk B supergiants. The observed variations inthe radial velocities, transient appearance of emission componentsin hydrogen line profiles and doublingof O I lines at 7774 Å support the possibility of this star beinga pulsating variable or a binary star.

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Observation and Astrometry data

Constellation:Andromeda
Right ascension:01h39m58.15s
Declination:+41°40'00.3"
Apparent magnitude:6.852
Distance:173.913 parsecs
Proper motion RA:42.1
Proper motion Dec:-1.9
B-T magnitude:8.004
V-T magnitude:6.948

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 10132
TYCHO-2 2000TYC 2822-1216-1
USNO-A2.0USNO-A2 1275-00988784
HIPHIP 7767

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