Chemical abundances of β Cephei stars from low- and high-resolution UV spectra

Details Chemical abundances of β Cephei stars from low- and high-resolution UV spectra Chemical abundances of β Cephei stars from low- and high-resolution UV spectra

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..310..259d&link_type=abstract

Variable Stars in the Local Group, IAU Colloquium 193, Proceedings of the conference held 6-11 July, 2003 at Christchurch, New Z

Astronomy and Astrophysics

Astronomy

Scientific paper

We determined the stellar parameters (Teff, [m/H], θ)
and E(B-V) for all β Cephei stars observed during the IUE satellite
mission. All parameters were derived using an algorithmic procedure of
fitting theoretical flux distributions (Kurucz 1996) to the IUE
observations.

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