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Theoretical astrophysics: an introduction
A concise yet comprehensive introduction to the central theoretical concepts of modern astrophysics, presenting hydrodynamics, radiation, and stellar dynamics all in one textbook. Adopting a modular structure, the author illustrates a small number of fundamental physical methods and principles, whic...
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Lenguaje: | eng |
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Wiley-VCH
2013
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Acceso en línea: | http://cds.cern.ch/record/1606413 |
_version_ | 1780931680979124224 |
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author | Bartelmann, Matthias |
author_facet | Bartelmann, Matthias |
author_sort | Bartelmann, Matthias |
collection | CERN |
description | A concise yet comprehensive introduction to the central theoretical concepts of modern astrophysics, presenting hydrodynamics, radiation, and stellar dynamics all in one textbook. Adopting a modular structure, the author illustrates a small number of fundamental physical methods and principles, which are sufficient to describe and understand a wide range of seemingly very diverse astrophysical phenomena and processes. For example, the formulae that define the macroscopic behavior of stellar systems are all derived in the same way from the microscopic distribution function. This function it |
id | cern-1606413 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2013 |
publisher | Wiley-VCH |
record_format | invenio |
spelling | cern-16064132021-04-21T22:23:54Zhttp://cds.cern.ch/record/1606413engBartelmann, MatthiasTheoretical astrophysics: an introductionAstrophysics and AstronomyA concise yet comprehensive introduction to the central theoretical concepts of modern astrophysics, presenting hydrodynamics, radiation, and stellar dynamics all in one textbook. Adopting a modular structure, the author illustrates a small number of fundamental physical methods and principles, which are sufficient to describe and understand a wide range of seemingly very diverse astrophysical phenomena and processes. For example, the formulae that define the macroscopic behavior of stellar systems are all derived in the same way from the microscopic distribution function. This function itWiley-VCHoai:cds.cern.ch:16064132013 |
spellingShingle | Astrophysics and Astronomy Bartelmann, Matthias Theoretical astrophysics: an introduction |
title | Theoretical astrophysics: an introduction |
title_full | Theoretical astrophysics: an introduction |
title_fullStr | Theoretical astrophysics: an introduction |
title_full_unstemmed | Theoretical astrophysics: an introduction |
title_short | Theoretical astrophysics: an introduction |
title_sort | theoretical astrophysics: an introduction |
topic | Astrophysics and Astronomy |
url | http://cds.cern.ch/record/1606413 |
work_keys_str_mv | AT bartelmannmatthias theoreticalastrophysicsanintroduction |