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The Symbiotic Phenomenon - Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18-20, 1987 (Paperback, Softcover reprint of the original 1st ed. 1988) Loot Price: R1,495
Discovery Miles 14 950
The Symbiotic Phenomenon - Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland,...

The Symbiotic Phenomenon - Proceedings of the 103rd Colloquium of the International Astronomical Union, Held in Torun, Poland, August 18-20, 1987 (Paperback, Softcover reprint of the original 1st ed. 1988)

Joanna Mikolajewska, M. Friedjung, Scott J. Kenyon, Roberto Viotti

Series: Astrophysics and Space Science Library, 145

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Loot Price R1,495 Discovery Miles 14 950 | Repayment Terms: R140 pm x 12*

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Symbiotic stars were identified spectroscopically as M giants with a very strong He II 4686 emission line. After five decades of study by many astronomers, the first internatioinal meetings devoted to symbiotics were held at the University of Colorado (Boulder) and at the Haute Provence Observatory during the Summer of 1981. These conferences emphasized exciting new results obtained by modern satellite (EINSTEIN, IUE) and ground-based observatories. Although the vast majority of the participants were already fairly sure that symbiotics are almost certainly interacting binary systems, and not extremely peculiar single stars, it was not clear exactly which types of physical processes were needed to be invoked to explain their observed behaviour. Many were even worried that it might not be possible to clearly define a class of "symbiotic stars" , and thus establish a unique model applicable to any system. Since the publication of the Haute-Provence proceedings, our understanding of the physical processes occuring in symbiotic stars (and in related objects such as cataclysmic variables and compact planetary nebulae) has greatly improved. We now speak confidently of a "symbiotic phenomenon" , in which an evolved red giant and a hot companion object (usually thought to be an accreting main sequence star or a luminous white dwarf star) happily coexist.

General

Imprint: Springer
Country of origin: Netherlands
Series: Astrophysics and Space Science Library, 145
Release date: November 2011
First published: 1988
Editors: Joanna Mikolajewska • M. Friedjung • Scott J. Kenyon • Roberto Viotti
Dimensions: 235 x 155 x 20mm (L x W x T)
Format: Paperback
Pages: 380
Edition: Softcover reprint of the original 1st ed. 1988
ISBN-13: 978-9401078337
Categories: Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
LSN: 9401078335
Barcode: 9789401078337

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