Spectral analysis of the binary sdB star Feige 36

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

Spectral analysis of the binary sdB star Feige 36

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

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Abstract

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 language	English
Title of host publication	In: Procs of the 11th European Workshop on White Dwarfs, ASP Conference Series 169
Publisher	Astronomical Society of the Pacific
Pages	546-550
ISBN (Print)	1-886733-91-0
Publication status	Published - 1999

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@inproceedings{98a48ed61aa743b785ff1ad5a256a461,

title = "Spectral analysis of the binary sdB star Feige 36",

abstract = "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.",

author = "H. Edelmann and U. Heber and R. Napiwotzki and I.N. Reid and R. Saffer",

note = "Original paper can be found at: http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific",

year = "1999",

language = "English",

isbn = "1-886733-91-0",

pages = "546--550",

booktitle = "In: Procs of the 11th European Workshop on White Dwarfs, ASP Conference Series 169",

publisher = "Astronomical Society of the Pacific",

address = "United States",

}

TY - GEN

T1 - Spectral analysis of the binary sdB star Feige 36

AU - Edelmann, H.

AU - Heber, U.

AU - Napiwotzki, R.

AU - Reid, I.N.

AU - Saffer, R.

N1 - Original paper can be found at: http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the Pacific

PY - 1999

Y1 - 1999

N2 - 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.

AB - 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.

M3 - Conference contribution

SN - 1-886733-91-0

SP - 546

EP - 550

BT - In: Procs of the 11th European Workshop on White Dwarfs, ASP Conference Series 169

PB - Astronomical Society of the Pacific

ER -

Spectral analysis of the binary sdB star Feige 36

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