Eta Carinae and the Supernova Impostors:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
New York, NY [u.a.]
Springer
2012
|
| Schriftenreihe: | Astrophysics and Space Science Library
384 |
| Schlagworte: | |
| Online-Zugang: | TUM01 UBT01 Volltext |
| Beschreibung: | In 1965 Fritz Zwicky proposed a class of supernovae that he called "Type V", described as "excessively faint at maximum." There were only two members, SN1961v and eta Carinae. We now know that eta Carinae was not a true supernova, but if it were observed today in a distant galaxy we would call it a "supernova impostor." 170 years ago it experienced a "great eruption" lasting 20 years, expelling 10 solar masses or more, and survived. Eta Carinae is now acknowledged as the most massive, most luminous star in our region of the Galaxy, and it may be our only accessible example of a very massive star in a pre-supernova state. In this book the editors and contributing authors review its remarkable history, physical state of the star and its ejecta, and its continuing instability. Chapters also include its relation to other massive, unstable stars, the massive star progenitors of supernovae, and the "first" stars in the Universe. |
| Beschreibung: | 1 Online-Ressource |
| ISBN: | 9781461422754 |
| DOI: | 10.1007/978-1-4614-2275-4 |
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| 500 | |a In 1965 Fritz Zwicky proposed a class of supernovae that he called "Type V", described as "excessively faint at maximum." There were only two members, SN1961v and eta Carinae. We now know that eta Carinae was not a true supernova, but if it were observed today in a distant galaxy we would call it a "supernova impostor." 170 years ago it experienced a "great eruption" lasting 20 years, expelling 10 solar masses or more, and survived. Eta Carinae is now acknowledged as the most massive, most luminous star in our region of the Galaxy, and it may be our only accessible example of a very massive star in a pre-supernova state. In this book the editors and contributing authors review its remarkable history, physical state of the star and its ejecta, and its continuing instability. Chapters also include its relation to other massive, unstable stars, the massive star progenitors of supernovae, and the "first" stars in the Universe. | ||
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Datensatz im Suchindex
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| geographic | Carinae Eta (DE-588)4342628-1 gnd |
| geographic_facet | Carinae Eta |
| id | DE-604.BV040751114 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T00:33:08Z |
| institution | BVB |
| isbn | 9781461422754 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-025730866 |
| oclc_num | 798968114 |
| open_access_boolean | |
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| owner_facet | DE-703 DE-91 DE-BY-TUM |
| physical | 1 Online-Ressource |
| psigel | ZDB-2-PHA |
| publishDate | 2012 |
| publishDateSearch | 2012 |
| publishDateSort | 2012 |
| publisher | Springer |
| record_format | marc |
| series | Astrophysics and Space Science Library |
| series2 | Astrophysics and Space Science Library |
| spelling | Davidson, Kris Verfasser aut Eta Carinae and the Supernova Impostors Kris Davidson ; Roberta M. Humphreys, ed. New York, NY [u.a.] Springer 2012 1 Online-Ressource txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library 384 In 1965 Fritz Zwicky proposed a class of supernovae that he called "Type V", described as "excessively faint at maximum." There were only two members, SN1961v and eta Carinae. We now know that eta Carinae was not a true supernova, but if it were observed today in a distant galaxy we would call it a "supernova impostor." 170 years ago it experienced a "great eruption" lasting 20 years, expelling 10 solar masses or more, and survived. Eta Carinae is now acknowledged as the most massive, most luminous star in our region of the Galaxy, and it may be our only accessible example of a very massive star in a pre-supernova state. In this book the editors and contributing authors review its remarkable history, physical state of the star and its ejecta, and its continuing instability. Chapters also include its relation to other massive, unstable stars, the massive star progenitors of supernovae, and the "first" stars in the Universe. Physics Astronomy Astronomy, Astrophysics and Cosmology Carinae Eta (DE-588)4342628-1 gnd rswk-swf Carinae Eta (DE-588)4342628-1 g DE-604 Humphreys, Roberta M. Sonstige oth Erscheint auch als Druckausgabe 978-1-4614-2274-7 Astrophysics and Space Science Library 384 (DE-604)BV041546891 384 https://doi.org/10.1007/978-1-4614-2275-4 Verlag Volltext |
| spellingShingle | Davidson, Kris Eta Carinae and the Supernova Impostors Astrophysics and Space Science Library Physics Astronomy Astronomy, Astrophysics and Cosmology |
| subject_GND | (DE-588)4342628-1 |
| title | Eta Carinae and the Supernova Impostors |
| title_auth | Eta Carinae and the Supernova Impostors |
| title_exact_search | Eta Carinae and the Supernova Impostors |
| title_full | Eta Carinae and the Supernova Impostors Kris Davidson ; Roberta M. Humphreys, ed. |
| title_fullStr | Eta Carinae and the Supernova Impostors Kris Davidson ; Roberta M. Humphreys, ed. |
| title_full_unstemmed | Eta Carinae and the Supernova Impostors Kris Davidson ; Roberta M. Humphreys, ed. |
| title_short | Eta Carinae and the Supernova Impostors |
| title_sort | eta carinae and the supernova impostors |
| topic | Physics Astronomy Astronomy, Astrophysics and Cosmology |
| topic_facet | Physics Astronomy Astronomy, Astrophysics and Cosmology Carinae Eta |
| url | https://doi.org/10.1007/978-1-4614-2275-4 |
| volume_link | (DE-604)BV041546891 |
| work_keys_str_mv | AT davidsonkris etacarinaeandthesupernovaimpostors AT humphreysrobertam etacarinaeandthesupernovaimpostors |