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Post-AGB Objects as a Phase of Stellar Evolution: 265 - R. Szczerba, S.K. Górny
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Post-AGB Objects as a Phase of Stellar Evolution: 265 - nieuw boek

2010, ISBN: 9048157587

Capa comum, [EAN: 9789048157587], Springer, Springer, Book, [PU: Springer], 2010-12-08, Springer, The term proto-planetary nebulae (PPNe) in the context of the late stages of stellar evol… Meer...

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Post-AGB Objects as a Phase of Stellar Evolution - pocketboek

2010, ISBN: 9789048157587

The term proto-planetary nebulae (PPNe), in the context of the late stages of stellar evolution, was created just over 20 years ago, to express the belief that in the near future these ob… Meer...

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Post-AGB Objects as a Phase of Stellar Evolution - pocketboek

2010

ISBN: 9789048157587

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Erscheinungsdatum: 08.12.2010, Medium: Taschenbuch, Einband: Kartoniert / Broschiert, Titel: Post-AGB Objects as a Phase of Stellar Evolution, Auflage: Softcover reprint of hardcover 1st … Meer...

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Post-AGB Objects as a Phase of Stellar Evolution - pocketboek

2001, ISBN: 9048157587

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Post-AGB Objects as a Phase of Stellar Evolution ab 200.49 EURO Astrophysics and Space Science Library. Softcover reprint of hardcover 1st ed. 2001 Medien > Bücher

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Post-AGB Objects as a Phase of Stellar Evolution - pocketboek

2010, ISBN: 9789048157587

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Softcover reprint of hardcover 1st ed. 2001, Softcover, Buch, [PU: Springer]

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Post-AGB Objects as a Phase of Stellar Evolution: 265

The term proto-planetary nebulae (PPNe), in the context of the late stages of stellar evolution, was created just over 20 years ago, to express the belief that in the near future these objects will become planetary nebulae (PNe). The first proto-planetary nebulae (also called post-Asymptotic Giant Branch or post-AGB objects) were discovered in the mid-1970s in the course of the Air Force Sky Survey. Investigation of this phase of stellar evolution developed very rapidly in the 1980s after the IRAS mission when it became clear that proto-planetary nebulae emit a significant part of their energy in the mid- and far-infrared. A new impetus in this field began in the 1990s with high spatial resolution imaging in mid-infrared and optical wavelengths. Evidence has been found that proto-planetary nebulae (at least their central parts) are quite asymmetric while shells of AGB stars display spherical shapes. The most intriguing challenge now is to understand which physical processes are dominant during formation and evolution of proto-planetary nebulae. Is it magnetic field, evolution in binary systems, planets, axisymmetric superwind mass loss and its further shaping by fast wind, collimated jets interacting with a spherically symmetric AGB remnant or maybe an interplay between these different processes? Another challenge is to explain why the mass loss process near the end of the AGB evolution is modulated on timescales of a few hundred years. The model presented during this workshop seems to be very promising in this respect.

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EAN (ISBN-13): 9789048157587
ISBN (ISBN-10): 9048157587
Gebonden uitgave
pocket book
Verschijningsjaar: 2010
Uitgever: Springer
472 Bladzijden
Gewicht: 0,707 kg
Taal: eng/Englisch

Boek bevindt zich in het datenbestand sinds 2011-07-15T19:32:14+02:00 (Amsterdam)
Detailpagina laatst gewijzigd op 2020-01-29T12:59:54+01:00 (Amsterdam)
ISBN/EAN: 9789048157587

ISBN - alternatieve schrijfwijzen:
90-481-5758-7, 978-90-481-5758-7


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