Stellar collapse - Info and Reading Options
By Chris L. Fryer

"Stellar collapse" was published by Kluwer Academic Publishers in 2004 - Dordrecht, it has 406 pages and the language of the book is English.
“Stellar collapse” Metadata:
- Title: Stellar collapse
- Author: Chris L. Fryer
- Language: English
- Number of Pages: 406
- Publisher: Kluwer Academic Publishers
- Publish Date: 2004
- Publish Location: Dordrecht
- Dewey Decimal Classification: 523.8/4465
- Library of Congress Classification: QB843.S95 S74 2004QB4-4.9QB4
“Stellar collapse” Subjects and Themes:
- Subjects: ➤ Gravitational collapse - Supernovae - Stars - Physics - Observations and Techniques Astronomy - Astrophysics and Astroparticles - Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences
Edition Specifications:
- Pagination: xxxi, 406 p. :
Edition Identifiers:
- The Open Library ID: OL19291602M - OL19509721W
- Online Computer Library Center (OCLC) ID: 55008255
- Library of Congress Control Number (LCCN): 2004047567
- ISBN-10: 1402019920 - 0306485990
- All ISBNs: 1402019920 - 0306485990
AI-generated Review of “Stellar collapse”:
"Stellar collapse" Description:
The Open Library:
Supernovae, hypernovae and gamma-ray bursts are among the most energetic explosions in the universe. The light from these outbursts is, for a brief time, comparable to billions of stars and can outshine the host galaxy within which the explosions reside. Most of the heavy elements in the universe are formed within these energetic explosions. Surprisingly enough, the collapse of massive stars is the primary source of not just one, but all three of these explosions. As all of these explosions arise from stellar collapse, to understand one requires an understanding of the others. Stellar Collapse marks the first book to combine discussions of all three phenomena, focusing on the similarities and differences between them. Designed for graduate students and scientists newly entering this field, this book provides a review not only of these explosions, but the detailed physical models used to explain them from the numerical techniques used to model neutrino transport and gamma-ray transport to the detailed nuclear physics behind the evolution of the collapse to the observations that have led to these three classes of explosions.
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