From luminous hot stars to starburst galaxies:
Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed intro...
Gespeichert in:
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Weitere beteiligte Personen: | , |
Format: | E-Book |
Sprache: | Englisch |
Veröffentlicht: |
Cambridge
Cambridge University Press
2008
|
Schriftenreihe: | Cambridge astrophysics
45 |
Links: | https://doi.org/10.1017/CBO9780511536199 |
Zusammenfassung: | Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution. |
Umfang: | 1 Online-Ressource (xiii, 315 Seiten) |
ISBN: | 9780511536199 |
Internformat
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spelling | Conti, P. S. From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer Cambridge Cambridge University Press 2008 1 Online-Ressource (xiii, 315 Seiten) txt c cr Cambridge astrophysics 45 Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution. Crowther, Paul A. Leitherer, Claus Erscheint auch als Druck-Ausgabe 9780521791342 Erscheint auch als Druck-Ausgabe 9781107407732 |
spellingShingle | Conti, P. S. From luminous hot stars to starburst galaxies |
title | From luminous hot stars to starburst galaxies |
title_auth | From luminous hot stars to starburst galaxies |
title_exact_search | From luminous hot stars to starburst galaxies |
title_full | From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer |
title_fullStr | From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer |
title_full_unstemmed | From luminous hot stars to starburst galaxies Peter S. Conti, Paul A. Crowther, Claus Leitherer |
title_short | From luminous hot stars to starburst galaxies |
title_sort | from luminous hot stars to starburst galaxies |
work_keys_str_mv | AT contips fromluminoushotstarstostarburstgalaxies AT crowtherpaula fromluminoushotstarstostarburstgalaxies AT leithererclaus fromluminoushotstarstostarburstgalaxies |