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: UNSPECIFIED.

Copy

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	Conference or Workshop Item (Other)
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	10 Jul 2025 23:21