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Meynet, G, Ekstrom, S, Maeder, A, Hirschi, R, Georgy, C and Beffa, C (2007) Developments in physics of massive stars. Proceedings of the International Astronomical Union, 3 (S250). pp. 147-160. ISSN 1743-9221
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0802.2805v1.pdf - Accepted Version
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Official URL: http://dx.doi.org/10.1017/S1743921308020449
Abstract
New constraints on stellar models are provided by large surveys of massive stars, interferometric observations and asteroseismology. After a review of the main results so far obtained, we present new results from rotating models and discuss comparisons with observed features. We conclude that rotation is a key feature of massive star physics.
Item Type: | Article |
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Additional Information: | This is the accepted author manuscript (AAM). The final published version (version of record) is available online via Cambridge University Press at http://dx.doi.org/10.1017/S1743921308020449 - please refer to any applicable terms of use of the publisher. |
Uncontrolled Keywords: | . stars: abundances, early-type, evolution, mass loss, emission-line, Be, rotation; gamma rays: bursts |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
Divisions: | Faculty of Natural Sciences > School of Physical and Geographical Sciences |
Related URLs: | |
Depositing User: | Symplectic |
Date Deposited: | 13 Dec 2016 12:11 |
Last Modified: | 12 Mar 2021 11:54 |
URI: | https://eprints.keele.ac.uk/id/eprint/2641 |
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