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Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
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Cataclysmic Variables and Related Objects - Proceedings of the 158th Colloquium of the International Astronomical Union, Held at Keele, United Kingdom, June 26-30, 1995 (Paperback, Softcover reprint of the original 1st ed. 1996)
Loot Price: R2,717
Discovery Miles 27 170
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Cataclysmic Variables and Related Objects - Proceedings of the 158th Colloquium of the International Astronomical Union, Held at Keele, United Kingdom, June 26-30, 1995 (Paperback, Softcover reprint of the original 1st ed. 1996)
Series: Astrophysics and Space Science Library, 208
Expected to ship within 18 - 22 working days
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In 1993 we began to consider the possibility of holding a
conference on Catacysmic Variables (CVs) at Keele University. There
have been several meetings in the area of CVs recently (e. g.
Eilat, Abano-Padova, Capetown). However as preparations for the
Keele meeting progressed we realized that, while there had been a
number of IAU meetings devoted to related and to peripheral topics
(such as IAU Colloquium 122 on Classical Novae in 1989, IAU
Colloquium 129 on Accretion Disks in 1990), there had been no
IAU-sponsored conferences in the area of cataclysmi/: variables
(CVs) for a number of years. We felt therefore that the time was
ripe to have an IAU meeting de voted to an overview of CVs and
related objects and the SOC organized the conference such that
there was an emphasis on invited reviews of the most recent
advances in the field. The conference covered both CVs and LMXBs
and the inter-relations between them. The meeting was held at a
time when powerful satellite observatories, and rapid improvements
in ground based instrumentation, had led to many advances in both
CV and LMXB research. The conference provided a forum to review
observations from ASCA, EUVE, ROSAT, Ginga and the
recently-refurbished HST. Photo metric, spectroscopic and
polarimetric observations of CVs and LMXBs have thrown new light on
the distribution of matter and the nature of the stellar components
in these systems.
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