Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...224...65c&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 224, no. 1-2, Oct. 1989, p. 65-72. Research supported by SERC.
Astronomy and Astrophysics
Astrophysics
21
B Stars, Blue Stars, Early Stars, Halos, Peculiar Stars, Abundance, Helium, Metallicity, Stellar Atmospheres
Scientific paper
High resolution optical spectra of eight high latitude blue stars have been obtained. Three of the sample are identified as subdwarfs. The remaining five are analyzed for atmospheric parameters and metal and He abundances using model atmosphere techniques. Four of the sample appear to be normal B type stars 2 kpc or more from the plane. With a logarithmic surface gravity estimated to be 4.6 + or - 0.3 dex, PB 166 could be either a main sequence, horizontal branch or cool subdwarf. The nature of this star is discussed in view of its approximately normal Population I chemical composition.
Brown Paul J. F.
Conlon E. S.
Dufton Philip L.
Keenan Francis P.
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