Spectral analysis of the binary sdB star Feige 36

H. Edelmann, U. Heber, R. Napiwotzki, I.N. Reid, R. Saffer

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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The sdB stars Feige 36 is a short-period, single-lined spectroscopic binary. Aymospheric parameters and abundances are determined from high-resolution Keck spectra. Feige 36 lies near the zero-age extreme Horizontal Branch position in the HRD.
Original languageEnglish
Title of host publicationIn: Procs of the 11th European Workshop on White Dwarfs, ASP Conference Series 169
PublisherAstronomical Society of the Pacific
ISBN (Print)1-886733-91-0
Publication statusPublished - 1999


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