Analysis of high-latitude blue stars. VI

Details Analysis of high-latitude blue stars. VI Analysis of high-latitude blue stars. VI

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.258...57k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 258, no. 1, Sept. 1, 1992, p. 57-63.

Other

32

Blue Stars, Milky Way Galaxy, Stellar Spectrophotometry, Stellar Magnitude, Subdwarf Stars

Scientific paper

Reticon spectroscoy at 50 and 100 A/mm and Stromgren uvby photometry are used to determine Teff, log g and V sin i for a sample of stars from the Luminous Stars in the Northern Milky Way catalogue and several 'faint blue star' catalogues. Four hot subdwarfs (and one probable hot subdwarf) are discovered, two of them helium-rich. Four other stars, apparently of Population I, are found to be helium-rich and three stars, including two of the helium-rich stars, appear to have distances from the galactic plane greater than 4 kpc.

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