Chemical abundances of β Cephei stars from low - and high - resolution UV spectra
نویسنده
چکیده
We determined 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 by using an algorithmic procedure of fitting theoretical flux distribution (Kurucz 1996) to the IUE observations.
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تاریخ انتشار 2004