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Condition: New.
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Language: English
Published by San Francisco, Astronomical Society of the Pacific,, 1993
First Edition
Gr.-8°, original hardcover. 1. ed. With numerous images, VIII, 156 p. Shelfmark on spine, stamp on title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.
Hardback. Condition: New.
Hardback. Condition: New.
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Language: English
Published by Astronomical Society of the Paci, 1993
ISBN 10: 0937707589 ISBN 13: 9780937707586
Seller: Bookmans, Tucson, AZ, U.S.A.
Hardcover. Condition: Good. No dust jacket. Satisfaction 100% guaranteed.
Seller: Ria Christie Collections, Uxbridge, United Kingdom
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Seller: Ria Christie Collections, Uxbridge, United Kingdom
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Seller: Books Puddle, New York, NY, U.S.A.
Condition: New. pp. 340.
Seller: Books Puddle, New York, NY, U.S.A.
Condition: New. pp. 340.
Language: English
Published by Springer New York, Springer US, 2012
ISBN 10: 1461422744 ISBN 13: 9781461422747
Seller: AHA-BUCH GmbH, Einbeck, Germany
Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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 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.
Seller: AHA-BUCH GmbH, Einbeck, Germany
Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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 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.
Seller: Mispah books, Redhill, SURRE, United Kingdom
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Seller: Revaluation Books, Exeter, United Kingdom
Hardcover. Condition: Brand New. 2012 edition. 339 pages. 9.75x6.50x0.75 inches. In Stock.
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Seller: PBShop.store UK, Fairford, GLOS, United Kingdom
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Add to basketHRD. Condition: New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.
Seller: Majestic Books, Hounslow, United Kingdom
Condition: New. Print on Demand pp. 212.
Seller: Books Puddle, New York, NY, U.S.A.
Condition: New. Print on Demand pp. 212.
Seller: Biblios, Frankfurt am main, HESSE, Germany
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Seller: AHA-BUCH GmbH, Einbeck, Germany
Buch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Studies on the populations of luminous stars in nearby resolved galaxies have revealed a complex distribution in the luminosity-temperature plane (the HR diagram). The fundamentals of massive star evolution are mostly understood, but the roles of mass loss, episodic mass loss, rotation, and binarity are still in question. Moreover, the final stages of these stars of different masses and their possible relation to each other are not understood. The purpose of this volume is to provide a current review of the different populations of evolved massive stars. The emphasis is on massive stars in the Local Group, the Magellanic Clouds, and the nearby spirals M31 and M33.
Seller: moluna, Greven, Germany
Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. KlappentextrnrnStudies on the populations of luminous stars in nearby resolved galaxies have revealed a complex distribution in the luminosity-temperature plane (the HR diagram). The fundamentals of massive star evolution are mostly understood, .