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Orbital solutions for the A-type binaries $\alpha$ Dra and Mizar A using spectrum disentangling

Published online by Cambridge University Press:  02 March 2005

A. Budovičová
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondřejov, Czech Republic email: andrea@asu.cas.cz
J. Kubát
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondřejov, Czech Republic email: andrea@asu.cas.cz
P. Hadrava
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondřejov, Czech Republic email: andrea@asu.cas.cz
M. šlechta
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondřejov, Czech Republic email: andrea@asu.cas.cz
D. Korčáková
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondřejov, Czech Republic email: andrea@asu.cas.cz
M. Dovčiak
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondřejov, Czech Republic email: andrea@asu.cas.cz
P. škoda
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondřejov, Czech Republic email: andrea@asu.cas.cz
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Abstract

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The single-lined 51.420d spectroscopic binary $\alpha$ Dra (HD 123299, Thuban, spectral type A0 III) is a slightly metal poor star. First orbital elements were obtained by Harper in 1907. Mizar A (HD 116656, spectral type A2 V) is a double-lined 20.53 d spectroscopic binary first reported by Pickering in 1890. Its orbital elements were determined by Vogel in 1901. The redetermination of the orbital elements for these two binaries used the spectrum disentangling computer code KOREL (Hadrava 1995, 1997). We present revised orbital elements based on new electronic spectra taken at the Ondřejov Observatory between 1994 and 2003.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2004 International Astronomical Union