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Astron. Astrophys. 364, L85-L88 (2000)
Letter to the Editor
Properties and nature of Be stars
XX. Binary nature and orbital elements of
Cas
P. Harmanec 1,2,
P. Habuda 3,
S. tefl 2,
P. Hadrava 2,
D. Kor áková 4,2,
P. Koubský 2,
J. Krti ka 4,2,
J. Kubát 2,
P. koda 2,
M. lechta 2 and
M. Wolf 1
1 Astronomical Institute of the Charles University, V Hole ovi kách 2, 180 00 Praha 8, Czech Republic
2 Astronomical Institute of the Academy of Sciences, 251 65 Ond ejov, Czech Republic
3 Faculty of Mathematics and Physics of the Charles University, Ke Karlovu 3, 121 16 Praha 2, Czech Republic
4 Masaryk University, Faculty of Science, Department of Theoretical Physics and Astrophysics, 611 37 Brno, Czech Republic
Received 20 September 2000 / Accepted 27 November 2000
Abstract
An analysis of accurate radial velocities (RVs) of the Be star
Cas from 295 Reticon
spectrograms secured between October 1993 and May 2000 allowed us to
prewhiten the RVs for the long-term changes and to obtain the first
orbital RV curve of this star. The orbital period is
203 59 and the orbit has an
eccentricity of 0.26. The orbital motion is de- tectable even in the
published velocities, based on photographic spectra. This implies that
Cas is a primary component of a
spectroscopic binary. The secondary has a mass of about
1 , appropriate for a white dwarf
or a neutron star, but it could also be a normal late-type dwarf. The
ultimate solution of the dispute whether the observed X-ray emission
is associated with the secondary or with the primary will need further
dedicated studies.
Key words: stars: binaries:
spectroscopic
stars: emission-line,
Be
stars: individual: fl Cas
Send offprint requests to: P. Harmanec (hec@sunstel.asu.cas.cz)
SIMBAD Objects
Contents
© European Southern Observatory (ESO) 2000
Online publication: January 29, 2001
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