Query : 2014A&A...570A...4C

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 - 2024
1 V* RS Oph Sy* 17 50 13.1591484960 -06 42 28.480729788   11.884 10.776 11.228   K5.5/M0IIIe 1092 0
2 V* V339 Del No* 20 23 30.6864752010 +20 46 03.777415270   17.50 16.86     ~ 204 0

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