Galaxies, structure and evolution:
Galaxies are large systems of stars, some of which contain interstellar gas and dust. They also contain much invisible matter, which may be in the form of weakly interacting elementary particles. In this introductory textbook, the first chapter introduces the study of galaxies. This is followed by t...
Gespeichert in:
| 1. Verfasser: | |
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| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Cambridge
Cambridge University Press
1993
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| Schlagworte: | |
| Online-Zugang: | BSB01 FHN01 Volltext |
| Zusammenfassung: | Galaxies are large systems of stars, some of which contain interstellar gas and dust. They also contain much invisible matter, which may be in the form of weakly interacting elementary particles. In this introductory textbook, the first chapter introduces the study of galaxies. This is followed by two chapters on observations of galaxies, including our own. There are then three chapters on galactic structure: the manner in which motions of stars determine galactic shape, the determination of galactic masses, and the structure of discs in spirals. Galactic evolution, especially changes in chemical composition over time, is covered. The book concludes with a discussion of the origin of galaxies and their relation to more general questions in cosmology. The book includes mathematical presentation where this enables the discussion to be quantitative |
| Beschreibung: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Beschreibung: | 1 online resource (xiii, 208 pages) |
| ISBN: | 9781139168137 |
| DOI: | 10.1017/CBO9781139168137 |
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| 520 | |a Galaxies are large systems of stars, some of which contain interstellar gas and dust. They also contain much invisible matter, which may be in the form of weakly interacting elementary particles. In this introductory textbook, the first chapter introduces the study of galaxies. This is followed by two chapters on observations of galaxies, including our own. There are then three chapters on galactic structure: the manner in which motions of stars determine galactic shape, the determination of galactic masses, and the structure of discs in spirals. Galactic evolution, especially changes in chemical composition over time, is covered. The book concludes with a discussion of the origin of galaxies and their relation to more general questions in cosmology. The book includes mathematical presentation where this enables the discussion to be quantitative | ||
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Datensatz im Suchindex
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| author | Tayler, R. J. |
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| ctrlnum | (ZDB-20-CBO)CR9781139168137 (OCoLC)992921299 (DE-599)BVBBV043943403 |
| dewey-full | 523.1/12 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1/12 |
| dewey-search | 523.1/12 |
| dewey-sort | 3523.1 212 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1017/CBO9781139168137 |
| format | Electronic eBook |
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| id | DE-604.BV043943403 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:39:19Z |
| institution | BVB |
| isbn | 9781139168137 |
| language | English |
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| oclc_num | 992921299 |
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| physical | 1 online resource (xiii, 208 pages) |
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| publishDate | 1993 |
| publishDateSearch | 1993 |
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| publisher | Cambridge University Press |
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| spelling | Tayler, R. J. Verfasser aut Galaxies, structure and evolution Roger J. Tayler Cambridge Cambridge University Press 1993 1 online resource (xiii, 208 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) Galaxies are large systems of stars, some of which contain interstellar gas and dust. They also contain much invisible matter, which may be in the form of weakly interacting elementary particles. In this introductory textbook, the first chapter introduces the study of galaxies. This is followed by two chapters on observations of galaxies, including our own. There are then three chapters on galactic structure: the manner in which motions of stars determine galactic shape, the determination of galactic masses, and the structure of discs in spirals. Galactic evolution, especially changes in chemical composition over time, is covered. The book concludes with a discussion of the origin of galaxies and their relation to more general questions in cosmology. The book includes mathematical presentation where this enables the discussion to be quantitative Galaxies Galaxies / Evolution Galaxie (DE-588)4057375-8 gnd rswk-swf Galaxie (DE-588)4057375-8 s 1\p DE-604 Erscheint auch als Druckausgabe 978-0-521-36431-7 Erscheint auch als Druckausgabe 978-0-521-36710-3 https://doi.org/10.1017/CBO9781139168137 Verlag URL des Erstveröffentlichers Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Tayler, R. J. Galaxies, structure and evolution Galaxies Galaxies / Evolution Galaxie (DE-588)4057375-8 gnd |
| subject_GND | (DE-588)4057375-8 |
| title | Galaxies, structure and evolution |
| title_auth | Galaxies, structure and evolution |
| title_exact_search | Galaxies, structure and evolution |
| title_full | Galaxies, structure and evolution Roger J. Tayler |
| title_fullStr | Galaxies, structure and evolution Roger J. Tayler |
| title_full_unstemmed | Galaxies, structure and evolution Roger J. Tayler |
| title_short | Galaxies, structure and evolution |
| title_sort | galaxies structure and evolution |
| topic | Galaxies Galaxies / Evolution Galaxie (DE-588)4057375-8 gnd |
| topic_facet | Galaxies Galaxies / Evolution Galaxie |
| url | https://doi.org/10.1017/CBO9781139168137 |
| work_keys_str_mv | AT taylerrj galaxiesstructureandevolution |