| Issue |
A&A
Volume 582, October 2015
|
|
|---|---|---|
| Article Number | A108 | |
| Number of page(s) | 4 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/201526882 | |
| Published online | 20 October 2015 | |
Mass fluxes for O-type supergiants with metallicity Z = Z⊙/5
Astrophysics Group, Blackett Laboratory, Imperial College London,
Prince Consort
Road
London
SW7 2AZ
UK
e-mail:
l.lucy@imperial.ac.uk
Received: 3 July 2015
Accepted: 3 September 2015
A code used previously to predict O-star mass fluxes as a function of metallicity is used to compute a grid of models with the metallicity of the Small Magellanic Cloud (SMC). These models allow mass-loss rates to be derived by interpolation for all O-type supergiants in the SMC, with the possible exception of extremely massive stars close to the Eddington limit.
Key words: stars: early-type / stars: mass-loss / stars: winds, outflows
© ESO, 2015
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