SIMBAD references

2005A&A...437..929C - Astronomy and Astrophysics, volume 437929-933 (2005/7-3)

Outflowing disk formation in B[e] supergiants due to rotation and bi-stability in radiation driven winds.

CURE M., RIAL D.F. and CIDALE L.

Abstract (from CDS):

The effects of rapid rotation and bi-stability upon the density contrast between the equatorial and polar directions of a B[e] supergiant are re-investigated. Based on a new slow solution for different high rotational radiation-driven winds and the fact that bi-stability allows a change in the line-force parameters (α, k, and δ), the equatorial densities are about 10²-10⁴ times higher than the polar ones. These values are in qualitative agreement with the observations.

Abstract Copyright: ∼

Journal keyword(s): stars: early-type - stars: mass-loss - stars: rotation - stars: winds, outflows

Simbad objects: 1

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