C.D.S. - SIMBAD4 rel 1.7 - 2021.04.22CEST05:39:59

2006A&A...450..219P - Astronomy and Astrophysics, volume 450, 219-225 (2006/4-4)

Are luminous and metal-rich Wolf-Rayet stars inflated?


Abstract (from CDS):

We investigate the influence of metallicity and stellar wind mass loss on the radius of Wolf-Rayet stars. We have calculated chemically homogeneous models of Wolf-Rayet stars of 10 to 200M for two metallicities (Z=0.02 and Z=0.001), without mass loss, using OPAL opacities. We also constructed theoretical helium main sequences for 15, 18, 24 and 30M with stellar wind mass loss rates of 10–5M/yr and 10–4M/yr and models for a 24M star for a few intermediate values of mass loss rate. We confirm the radius extension for luminous, metal-rich Wolf-Rayet stars reported previously by Ishii et al. (1999PASJ...51..417I), i.e. the inflation of the hydrostatic stellar radius. We also show that for small values of the stellar wind mass loss rate, an extended envelope structure is still present. However, for mass loss rates above a critical value, for which we derive an expression, Wolf-Rayet radii decrease and the stellar structure becomes compact. We briefly discuss possible evolutionary and observational consequences of an inflated envelope for a mass losing Wolf-Rayet star.

Abstract Copyright:

Journal keyword(s): stars: fundamental parameters - stars: Wolf-Rayet - stars: interiors - stars: mass-loss - stars: winds, outflows

Simbad objects: 2

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Number of rows : 2

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
1 HD 226868 HXB 19 58 21.6758193269 +35 12 05.782512305 9.38 9.72 8.91 8.42   O9.7Iabpvar 3998 0
2 V* V1521 Cyg HXB 20 32 25.78 +40 57 27.9           WN4/5-6/7 1806 2

    Equat.    Gal    SGal    Ecl

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