Asymptotic Giant Branch Stars:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
New York, NY
Springer New York
2004
|
| Schriftenreihe: | Astronomy and Astrophysics Library
|
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | This book deals with stars during a short episode before they undergo a ma jor, and fatal, transition. Soon the star will stop releasing nudear energy, it will become a planetary nebula for abrief but poetic moment, and then it will turn into a white dwarf and slowly fade out of sight. Just before this dramatic change begins the star has reached the highest luminosity and the largest diameter in its existence, and while it is a star detectable in galaxies beyond the Local Group, its structure contains already the inconspicuous white dwarf it will become. It is called an "asymptotic giant branch star" or "AGB star". Over the last 30 odd years AGB stars have become a topic of their own although individual members of this dass had already been studied for cen turies without realizing what they were. In the early evolution, so called "E-AGB"-phase, the stars are a bit bluer than, but otherwise very similar to, what are now called red giant branch stars (RGB stars). It is only in the sec ond half of their anyhow brief existence that AGB stars differ fundamentally from RGB stars |
| Beschreibung: | 1 Online-Ressource (IX, 562 p) |
| ISBN: | 9781475738766 9781441918437 |
| ISSN: | 0941-7834 |
| DOI: | 10.1007/978-1-4757-3876-6 |
Internformat
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| 300 | |a 1 Online-Ressource (IX, 562 p) | ||
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| 500 | |a This book deals with stars during a short episode before they undergo a ma jor, and fatal, transition. Soon the star will stop releasing nudear energy, it will become a planetary nebula for abrief but poetic moment, and then it will turn into a white dwarf and slowly fade out of sight. Just before this dramatic change begins the star has reached the highest luminosity and the largest diameter in its existence, and while it is a star detectable in galaxies beyond the Local Group, its structure contains already the inconspicuous white dwarf it will become. It is called an "asymptotic giant branch star" or "AGB star". Over the last 30 odd years AGB stars have become a topic of their own although individual members of this dass had already been studied for cen turies without realizing what they were. In the early evolution, so called "E-AGB"-phase, the stars are a bit bluer than, but otherwise very similar to, what are now called red giant branch stars (RGB stars). It is only in the sec ond half of their anyhow brief existence that AGB stars differ fundamentally from RGB stars | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astronomy, Observations and Techniques | |
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Datensatz im Suchindex
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| discipline | Physik |
| doi_str_mv | 10.1007/978-1-4757-3876-6 |
| format | Electronic eBook |
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| id | DE-604.BV042412358 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:50Z |
| institution | BVB |
| isbn | 9781475738766 9781441918437 |
| issn | 0941-7834 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027847851 |
| oclc_num | 864054721 |
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| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (IX, 562 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 2004 |
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| publisher | Springer New York |
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| series2 | Astronomy and Astrophysics Library |
| spelling | Habing, Harm J. Verfasser aut Asymptotic Giant Branch Stars edited by Harm J. Habing, Hans Olofsson New York, NY Springer New York 2004 1 Online-Ressource (IX, 562 p) txt rdacontent c rdamedia cr rdacarrier Astronomy and Astrophysics Library 0941-7834 This book deals with stars during a short episode before they undergo a ma jor, and fatal, transition. Soon the star will stop releasing nudear energy, it will become a planetary nebula for abrief but poetic moment, and then it will turn into a white dwarf and slowly fade out of sight. Just before this dramatic change begins the star has reached the highest luminosity and the largest diameter in its existence, and while it is a star detectable in galaxies beyond the Local Group, its structure contains already the inconspicuous white dwarf it will become. It is called an "asymptotic giant branch star" or "AGB star". Over the last 30 odd years AGB stars have become a topic of their own although individual members of this dass had already been studied for cen turies without realizing what they were. In the early evolution, so called "E-AGB"-phase, the stars are a bit bluer than, but otherwise very similar to, what are now called red giant branch stars (RGB stars). It is only in the sec ond half of their anyhow brief existence that AGB stars differ fundamentally from RGB stars Physics Astronomy, Observations and Techniques Olofsson, Hans Sonstige oth https://doi.org/10.1007/978-1-4757-3876-6 Verlag Volltext |
| spellingShingle | Habing, Harm J. Asymptotic Giant Branch Stars Physics Astronomy, Observations and Techniques |
| title | Asymptotic Giant Branch Stars |
| title_auth | Asymptotic Giant Branch Stars |
| title_exact_search | Asymptotic Giant Branch Stars |
| title_full | Asymptotic Giant Branch Stars edited by Harm J. Habing, Hans Olofsson |
| title_fullStr | Asymptotic Giant Branch Stars edited by Harm J. Habing, Hans Olofsson |
| title_full_unstemmed | Asymptotic Giant Branch Stars edited by Harm J. Habing, Hans Olofsson |
| title_short | Asymptotic Giant Branch Stars |
| title_sort | asymptotic giant branch stars |
| topic | Physics Astronomy, Observations and Techniques |
| topic_facet | Physics Astronomy, Observations and Techniques |
| url | https://doi.org/10.1007/978-1-4757-3876-6 |
| work_keys_str_mv | AT habingharmj asymptoticgiantbranchstars AT olofssonhans asymptoticgiantbranchstars |