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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1. Verfasser: | |
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Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Cambridge
Cambridge University Press
1989
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Schlagworte: | |
Online-Zugang: | BSB01 FHN01 URL des Erstveröffentlichers |
Zusammenfassung: | 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 |
Beschreibung: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
Beschreibung: | 1 online resource (xi, 249 pages) |
ISBN: | 9780511623011 |
DOI: | 10.1017/CBO9780511623011 |
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245 | 1 | 0 | |a Introduction to stellar astrophysics, Volume 2, Stellar atmospheres |c Erika Böhm-Vitense |
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500 | |a Title from publisher's bibliographic system (viewed on 05 Oct 2015) | ||
520 | |a 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 | ||
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Datensatz im Suchindex
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any_adam_object | |
author | Böhm-Vitense, E. |
author_facet | Böhm-Vitense, E. |
author_role | aut |
author_sort | Böhm-Vitense, E. |
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dewey-full | 523.8 |
dewey-hundreds | 500 - Natural sciences and mathematics |
dewey-ones | 523 - Specific celestial bodies and phenomena |
dewey-raw | 523.8 |
dewey-search | 523.8 |
dewey-sort | 3523.8 |
dewey-tens | 520 - Astronomy and allied sciences |
discipline | Physik |
doi_str_mv | 10.1017/CBO9780511623011 |
format | Electronic eBook |
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illustrated | Not Illustrated |
indexdate | 2024-07-10T07:39:24Z |
institution | BVB |
isbn | 9780511623011 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029354883 |
oclc_num | 967605661 |
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owner | DE-12 DE-92 |
owner_facet | DE-12 DE-92 |
physical | 1 online resource (xi, 249 pages) |
psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
publishDate | 1989 |
publishDateSearch | 1989 |
publishDateSort | 1989 |
publisher | Cambridge University Press |
record_format | marc |
spelling | Böhm-Vitense, E. Verfasser aut Introduction to stellar astrophysics, Volume 2, Stellar atmospheres Erika Böhm-Vitense Cambridge Cambridge University Press 1989 1 online resource (xi, 249 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) 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 Stars Astrophysics Erscheint auch als Druckausgabe 978-0-521-34403-6 Erscheint auch als Druckausgabe 978-0-521-34870-6 https://doi.org/10.1017/CBO9780511623011 Verlag URL des Erstveröffentlichers Volltext |
spellingShingle | Böhm-Vitense, E. Introduction to stellar astrophysics, Volume 2, Stellar atmospheres Stars Astrophysics |
title | Introduction to stellar astrophysics, Volume 2, Stellar atmospheres |
title_auth | Introduction to stellar astrophysics, Volume 2, Stellar atmospheres |
title_exact_search | Introduction to stellar astrophysics, Volume 2, Stellar atmospheres |
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, Volume 2, Stellar atmospheres |
title_sort | introduction to stellar astrophysics volume 2 stellar atmospheres |
topic | Stars Astrophysics |
topic_facet | Stars Astrophysics |
url | https://doi.org/10.1017/CBO9780511623011 |
work_keys_str_mv | AT bohmvitensee introductiontostellarastrophysicsvolume2stellaratmospheres |