C.D.S. - SIMBAD4 rel 1.7 - 2021.01.16CET19:28:54

2014A&A...570A...4C - Astronomy and Astrophysics, volume 570A, 4-4 (2014/10-1)

The applicability of the wind compression model.


Abstract (from CDS):

Compression of the stellar winds from rapidly rotating hot stars is described by the wind compression model. However, it was also shown that rapid rotation leads to rotational distortion of the stellar surface, resulting in the appearance of non-radial forces acting against the wind compression. In this note we justify the wind compression model for moderately rotating white dwarfs and slowly rotating giants. The former could be conducive to understanding density/ionization structure of the mass outflow from symbiotic stars and novae, while the latter can represent an effective mass-transfer mode in the wide interacting binaries.

Abstract Copyright:

Journal keyword(s): stars: activity - 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 V* RS Oph No* 17 50 13.1592776879 -06 42 28.481553668   12.29 4.30     OB+M2ep 935 0
2 NOVA Del 2013 No* 20 23 30.6864752010 +20 46 03.777415270   17.50 16.86     ~ 161 0

    Equat.    Gal    SGal    Ecl

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