Spectral analysis of the binary sdB star Feige 36

Edelmann, H., Heber, U., Napiwotzki, R., Reid, I.N. and Saffer, R. (1999) Spectral analysis of the binary sdB star Feige 36. In: In: Procs of the 11th European Workshop on White Dwarfs, ASP Conference Series 169 :. Astronomical Society of the Pacific, pp. 546-550. ISBN 1-886733-91-0
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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.
Item Type Book Section
Additional information Original paper can be found at: http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific
Date Deposited 15 May 2025 16:18
Last Modified 30 May 2025 23:08

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