Astrophysics of Red Supergiants

Nonfiction, Science & Nature, Science, Physics, Astronomy
Cover of the book Astrophysics of Red Supergiants by Emily M Levesque, Institute of Physics Publishing
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Author: Emily M Levesque ISBN: 9780750313292
Publisher: Institute of Physics Publishing Publication: December 19, 2017
Imprint: Institute of Physics Publishing Language: English
Author: Emily M Levesque
ISBN: 9780750313292
Publisher: Institute of Physics Publishing
Publication: December 19, 2017
Imprint: Institute of Physics Publishing
Language: English

Astrophysics of Red Supergiants is the first book of its kind devoted to our current knowledge of red supergiant stars, a key evolutionary phase that is critical to our larger understanding of massive stars. The book provides a comprehensive overview of the fundamental physical properties of red supergiants, their evolution, and their extragalactic and cosmological applications. It serves as a reference for researchers from a broad range of fields (including stellar astrophysics, supernovae, and high-redshift galaxies) who are interested in red supergiants as extreme stages of stellar evolution, dust producers, supernova progenitors, extragalactic metallicity indicators, members of massive binaries and mergers, or simply as compelling objects in their own right. The book is accessible to a range of experience levels, from graduate students up to senior researchers.

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Astrophysics of Red Supergiants is the first book of its kind devoted to our current knowledge of red supergiant stars, a key evolutionary phase that is critical to our larger understanding of massive stars. The book provides a comprehensive overview of the fundamental physical properties of red supergiants, their evolution, and their extragalactic and cosmological applications. It serves as a reference for researchers from a broad range of fields (including stellar astrophysics, supernovae, and high-redshift galaxies) who are interested in red supergiants as extreme stages of stellar evolution, dust producers, supernova progenitors, extragalactic metallicity indicators, members of massive binaries and mergers, or simply as compelling objects in their own right. The book is accessible to a range of experience levels, from graduate students up to senior researchers.

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