Issue |
A&A
Volume 474, Number 3, November II 2007
|
|
---|---|---|
Page(s) | 701 - 706 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361:20078236 | |
Published online | 23 October 2007 |
The structure of line-driven winds
Astrophysics Group, Blackett Laboratory, Imperial College London, Prince Consort Road, London SW7 2AZ, UK e-mail: l.lucy@imperial.ac.uk
Received:
6
July
2007
Accepted:
11
September
2007
Following procedures pioneered by Castor et al. (1975, ApJ, 195, 157, [CAK]), spherically-symmetric supersonic winds for O stars are computed for matching to plane-parallel moving reversing layers (RL's) from Paper I (Lucy 2007, A&A, 468, 649). In contrast to a CAK wind, each of these solutions is singularity-free, thus allowing its mass-loss rate to be fixed by the regularity condition at the sonic point within the RL. Moreover, information propagation in these winds by radiative-acoustic waves is everywhere outwardly-directed, justifying the implicit assumption in Paper I that transonic flows are unaffected by inwardly-directed wave motions.
Key words: stars: early-type / stars: mass-loss / stars: winds, outflows
© ESO, 2007
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.