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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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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
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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