Issue |
A&A
Volume 434, Number 2, May I 2005
|
|
---|---|---|
Page(s) | 677 - 689 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20042061 | |
Published online | 11 April 2005 |
Understanding B-type supergiants in the low metallicity environment of the SMC II
1
The Isaac Newton Group of Telescopes, Apartado de Correos 321, 38700 Santa Cruz de La Palma, Canary Islands, Spain e-mail: ctrundle@iac.es
2
The Department of Pure and Applied Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland
Received:
24
September
2004
Accepted:
5
January
2005
Despite a resurgence of effort over the last decade in the area of
massive stars there is still ambiguity over their evolutionary path,
contamination of their surface abundances and the behaviour of their stellar
winds. Here 10 SMC B-type supergiants are analysed applying a unified model
atmosphere code fastwind to intermediate resolution spectra from the ESO
Multi Mode Instrument (emmi) on the NTT telescope. Combined with the 8
targets analysed in Paper I (Trundle et al. 2004), this work provides
observational results on the properties of the winds and chemical compositions
of B-type supergiants in the SMC. This paper emphasizes and substantiates
the implications for stellar evolution from Paper I; that current theoretical
models need to produce larger degrees of surface nitrogen enhancements at lower
rotational velocities. In addition a significant discrepancy between
theoretical and observed mass-loss rates is discussed which will have important
implications for the rotational velocities obtained from stellar evolution
calculations. Furthermore, an initial calibration of the wind-momentum
luminosity relationship for B-type supergiants in a low metallicity environment
() is presented.
Key words: stars: early-type / stars: supergiants / stars: mass-loss / stars: evolution / galaxies: Magellanic Clouds / cosmology: distance scale
© ESO, 2005
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