A&A 453, L35-L37 (2006)
DOI: 10.1051/0004-6361:200600027
Letter
A MOST probable explanation of the pulsation of WR 123
E. A. Dorfi1, A. Gautschy2 and H. Saio31 Institut für Astronomie der Universität Wien, Türkenschanzstr. 17, 1180 Wien, Austria
e-mail: dorfi@astro.univie.ac.at
2 Wetterchrüzstr. 8c, 4410 Liestal, Switzerland
3 Astronomical Institute, Tohoku University, Sendai, Japan
(Received 28 November 2005 / Accepted 18 May 2006 )
Abstract
Aims.Resorting to the observed period of the cyclic part of
WR 123's photometric variability we constrain its stellar
parameters.
Methods.Radiation hydrodynamic simulations were performed on
selected stellar envelope models for which also linear stability
analyses were computed.
Results.Pulsations of massive hydrogen-rich stellar envelopes
subject to sufficiently high luminosity-to-mass ratios
are excited with periods that conform with the observed
one by MOST in WR123.
Key words: stars: massive -- stars: pulsations -- stars: individual: WR123
© ESO 2006
BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook