Introduction to stellar astrophysics: Volume 2 Stellar atmospheres
This comprehensive textbook conveys the basic physical ideas and laws used in the study of the outer layers of a star. The stellar atmosphere emits the light which we see. The only layers of a star where we can get direct information about temperature, pressure and composition are in the atmosphere....
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| Main Author: | |
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| Format: | eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
1989
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| Links: | https://doi.org/10.1017/CBO9780511623011 |
| Summary: | This comprehensive textbook conveys the basic physical ideas and laws used in the study of the outer layers of a star. The stellar atmosphere emits the light which we see. The only layers of a star where we can get direct information about temperature, pressure and composition are in the atmosphere. This complete account first introduces stellar magnitudes, spectra and temperatures. This is followed by a full discussion of radiative transfer in a stellar atmosphere, which leads to descriptions of line formation, the spectrum of hydrogen, and spectral analysis. Finally the structural components that are accessible, such as the convestion zone, chromosphere, corona, and mass outflow are described. The book will interest any student with a knowledge of physics and mathematics who needs to learn about stellar atmospheres. |
| Physical Description: | 1 Online-Ressource (xi, 249 Seiten) |
| ISBN: | 9780511623011 |
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| id | ZDB-20-CTM-CR9780511623011 |
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| indexdate | 2025-03-19T15:54:05Z |
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| isbn | 9780511623011 |
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| spelling | Böhm-Vitense, E. Introduction to stellar astrophysics Volume 2 Stellar atmospheres Erika Böhm-Vitense Cambridge Cambridge University Press 1989 1 Online-Ressource (xi, 249 Seiten) txt c cr This comprehensive textbook conveys the basic physical ideas and laws used in the study of the outer layers of a star. The stellar atmosphere emits the light which we see. The only layers of a star where we can get direct information about temperature, pressure and composition are in the atmosphere. This complete account first introduces stellar magnitudes, spectra and temperatures. This is followed by a full discussion of radiative transfer in a stellar atmosphere, which leads to descriptions of line formation, the spectrum of hydrogen, and spectral analysis. Finally the structural components that are accessible, such as the convestion zone, chromosphere, corona, and mass outflow are described. The book will interest any student with a knowledge of physics and mathematics who needs to learn about stellar atmospheres. Erscheint auch als Druck-Ausgabe 9780521344036 Erscheint auch als Druck-Ausgabe 9780521348706 |
| spellingShingle | Böhm-Vitense, E. Introduction to stellar astrophysics |
| title | Introduction to stellar astrophysics |
| title_auth | Introduction to stellar astrophysics |
| title_exact_search | Introduction to stellar astrophysics |
| title_full | Introduction to stellar astrophysics Volume 2 Stellar atmospheres Erika Böhm-Vitense |
| title_fullStr | Introduction to stellar astrophysics Volume 2 Stellar atmospheres Erika Böhm-Vitense |
| title_full_unstemmed | Introduction to stellar astrophysics Volume 2 Stellar atmospheres Erika Böhm-Vitense |
| title_short | Introduction to stellar astrophysics |
| title_sort | introduction to stellar astrophysics stellar atmospheres |
| work_keys_str_mv | AT bohmvitensee introductiontostellarastrophysicsvolume2 |