A MOST probable explanation of the pulsation of WR 123

Details A MOST probable explanation of the pulsation of WR 123 A MOST probable explanation of the pulsation of WR 123

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...453l..35d&link_type=abstract

Astronomy and Astrophysics, Volume 453, Issue 3, July III 2006, pp.L35-L37

Astronomy and Astrophysics

Astrophysics

22

Stars: Massive, Stars: Pulsations, Stars: Individual: Wr123

Scientific paper

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.

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