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Massive Star Evolution

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 1999 Germany English Publisher:Cambridge University Press (CUP)Journal:Symposium - International Astronomical Union, volume 190, pages 192-199 (issn: 0074-1809,

Authors: Langer, Norbert; Heger, Alexander;

doi: 10.1017/s0074180900117838

Massive Star Evolution

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Abstract

The evolution of massive stars is far from being fully understood, as we outline by pointing to a number of open problems related to massive stars in the Magellanic Clouds. We argue that rotation may be a key ingredient in the physics of massive stars. We report on recent results obtained including rotation, and their relevance to these remaining questions.

Country

Germany

Related Organizations

University of Potsdam
Germany

Keywords

Institut für Physik und Astronomie

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	1
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average