Eta Carinae and the Supernova Impostors
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...
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| Главный автор: | |
|---|---|
| Другие авторы: | |
| Формат: | Livre numérique |
| Язык: | Anglais |
| Опубликовано: |
New York, NY :
Springer New York
[20..].
Cham : Springer Nature |
| Редактирование: | 1st ed. 2012. |
| Серии: | Astrophysics and Space Science Library
384 |
| Online-ссылка: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Примечание: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Eta Carinae and the supernova impostors, Kris Davidson, Roberta M. Humphreys, New York, Springer, 2012, 1 vol. (X-329 p.), Astrophysics and space science library, 978-1-4614-2274-7 • Eta Carinae and the Supernova Impostors, Texte imprimé, 9781489989253 • Eta Carinae and the Supernova Impostors, Texte imprimé, 9781461422761 |
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| 100 | 1 | |a Davidson, Kris. | |
| 245 | 1 | 0 | |a Eta Carinae and the Supernova Impostors |c edited by Kris Davidson, Roberta M. Humphreys. |
| 250 | |a 1st ed. 2012. | ||
| 260 | |a New York, NY : |b Springer New York. | ||
| 260 | |a Cham : |b Springer Nature, |c [20..]. | ||
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| 505 | 1 | |a Eta Carinae - From 1600 to the Present The Company Eta Carinae Keeps - Stellar and Interstellar Content of the Carina The Central Star - Instability and Recovery The Winds of Eta Carinae and Other Very Luminous Stars Physics of the Inner Ejecta High-resolution Studies of Eta Carinae's Ejecta and Stellar Wind All Things Homunculus The Outer Ejecta X-ray Variability and the Secondary Star Eta Carinae and the Luminous Blue Variables The Supernova Imposters Instability and Mass Loss Near the Eddington Limit The Final Struggles of Massive Star Evolution and Their Supernovae | |
| 506 | |a Accès en ligne pour les établissements français bénéficiaires des licences nationales | ||
| 506 | |a Accès soumis à abonnement pour tout autre établissement | ||
| 506 | |a Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. https://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 | ||
| 520 | |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 | ||
| 700 | 1 | |a Humphreys, Roberta M. |4 pbd | |
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| 776 | 0 | |t Eta Carinae and the Supernova Impostors |b Texte imprimé |z 9781489989253 | |
| 776 | 0 | |t Eta Carinae and the Supernova Impostors |b Texte imprimé |z 9781461422761 | |
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