The UV silicon spectra of early B stars

Details The UV silicon spectra of early B stars The UV silicon spectra of early B stars

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281a.393m&link_type=abstract

In ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1 p 393-396 (SEE N89-10682 01-89)

Astronomy and Astrophysics

Astronomy

1

B Stars, Iue, Silicon, Spaceborne Astronomy, Stellar Spectra, Ultraviolet Astronomy, Ultraviolet Spectra, Atomic Spectra, Emission Spectra, Spectral Line Width

Scientific paper

The UV silicon spectra of mid to early B stars are examined and compared
to models. It is found that lines are extremely sensitive to stellar
temperature and luminosity. Although the models fail to predict the
quantitative behavior of the line strengths, they do, in most instances,
describe their qualitative behavior.

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