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. Astronomical Society of the Pacific.

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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	Other
Divisions	?? sbu_spam ?? ?? sbu_specs ?? ?? dep_pam ??
Date Deposited	18 Nov 2024 12:27
Last Modified	18 Nov 2024 12:27

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