Wolf-Rayet stars as (potentially) fast rotators with rotationally-induced instability

Details Wolf-Rayet stars as (potentially) fast rotators with rotationally-induced instability Wolf-Rayet stars as (potentially) fast rotators with rotationally-induced instability

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221..169m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 169-180

Physics

3

Main Sequence Stars, Massive Stars, O Stars, Stellar Physics, Stellar Rotation, Stellar Systems, Stellar Winds, Wolf-Rayet Stars, Binary Stars, Solar Flares, Stellar Luminosity, Stellar Magnetic Fields, Stellar Mass, Stellar Models, Stellar Spectra

Scientific paper

Indirect lines of evidence for fast axial rotation of Wolf-Rayet (WR)
stars are described, such as 1) elongated cavities around WRs; 2)
flattening of WR winds; 3) solar-like flares of WRs; 4) non-radial
pulsations of the WR wind in the presence of a massive companion in a
binary system.

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