Analysis of high-latitude blue stars. II

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

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234.1011k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Oct. 15, 1988, p. 1011-1019.

Astronomy and Astrophysics

Astronomy

15

Blue Stars, Early Stars, Stellar Spectra, H Gamma Line, Helium, Line Spectra, O Stars, Stellar Luminosity

Scientific paper

A simple analysis of five high-latitude early-type stars is presented. Reticon spectra and Strömgren photometry are used to determine Teff and log g from "Kiel diagrams" and values of V sin i are estimated from He I lines. The results are checked by fitting Kurucz (1979) profiles to the observed Hγ and Hδ profiles. Four stars appear spectroscopically normal although one might be subluminous; implied distances from the galactic plane are between 3 and 15 kpc. One star, TONS 308, could be a spectrum variable.

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