From Twilight to Highlight: The Physics of Supernovae
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"From Twilight to Highlight: The Physics of Supernovae" by W. Hillebrandt (Ed) is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.
Supernovae, their bearing on cosmology and their connection to gamma-ray bursts are now at the center of astrophysical research programs. This volume deals with astronomical observations of supernovae and their relation to nuclear and particle astrophysics. All known aspects of supernovae explosions are investigated in articles specifically written for researchers and advanced graduate students. It also includes recent numerical "experiments" related to the question of hydrodynamical instability in two and three dimensions and to problems concerning the complexity of radiation transport in the models. Other contributions discuss the possible energy sources needed to drive these powerful stellar explosions.
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"From Twilight to Highlight: The Physics of Supernovae" by W. Hillebrandt (Ed) is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.
Topic: Deep Sky & Solar System
Author: W. Hillebrandt (Ed)
Who this is for:
- Astronomy students
- Researchers and advanced hobbyists
- Readers exploring space science topics
Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.
Supernovae, their bearing on cosmology and their connection to gamma-ray bursts are now at the center of astrophysical research programs. This volume deals with astronomical observations of supernovae and their relation to nuclear and particle astrophysics. All known aspects of supernovae explosions are investigated in articles specifically written for researchers and advanced graduate students. It also includes recent numerical "experiments" related to the question of hydrodynamical instability in two and three dimensions and to problems concerning the complexity of radiation transport in the models. Other contributions discuss the possible energy sources needed to drive these powerful stellar explosions.
| Author | W. Hillebrandt (Ed) |
| Publisher | Springer Science & Business Media |
| Published | 2003-02-27 |
| ISBN-13 | 9783540004837 |
| Binding | Hardcover |
| Pages | 446 |
| Language | English |
| Subjects | Science |
| Topic | Deep Sky & Solar System |
| Series | Eso Astrophysics Symposia |
Format: Hardcover
Length: 446 pages
Language: English
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