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Titlebook: Cataclysmic Variables; Proceedings of the C A. Bianchini,M. Della Valle,M. Orio Conference proceedings 1995 Springer Science+Business Media

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书目名称Cataclysmic Variables
副标题Proceedings of the C
编辑A. Bianchini,M. Della Valle,M. Orio
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Cataclysmic Variables; Proceedings of the C A. Bianchini,M. Della Valle,M. Orio Conference proceedings 1995 Springer Science+Business Media
描述Cataclysmic Variables (CVs) are well furnished laboratories in which one can investigate a number of important physical processes. These processes include: thermonuclear reactions, nebular physics, winds, mass accretion phenomena on compact objects, magnetohydrodynamics, plasmas, thermal and non thermal radiative processes, relativistic phenomena, dust forma­ tion, etc . . In the recent year the most exciting development in our opinion was that the small, cold and invisible secondary components of CV s were found to be the prime motors for the evolution of close binary systems, disclosing new scenarios for research. All branches of astronomy and as­ trophysics often take advantage of the new ideas brought by the study of CVs. It is for this reason, we believe, that meetings on CVs are important for most of the astronomical community. The idea of a Congress on CVs in Padova has been fluttering in the air for a few years. After all - we thought - a large part of the scientific heritage of Padova and Asiago Observatories is represented by the study of variable stars and, in particular, of CV s, as Prof. L. Rosino reminded us at the very beginning of the Congress. We finally chose Aban
出版日期Conference proceedings 1995
关键词Accretion; X-ray; nebula; physics
版次1
doihttps://doi.org/10.1007/978-94-011-0335-0
isbn_softcover978-94-010-4148-5
isbn_ebook978-94-011-0335-0Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1995
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How They Reduce Organizational Pain,I have been requested by Antonio Bianchini to say a few words at the beginning of this Conference to recall the work on cata clysmic variables carried out for about fifty years, at first at Loiano (Bologna), and after some years, at the Astrophysical Observatory at Asiago.
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Conference proceedings 1995lude: thermonuclear reactions, nebular physics, winds, mass accretion phenomena on compact objects, magnetohydrodynamics, plasmas, thermal and non thermal radiative processes, relativistic phenomena, dust forma­ tion, etc . . In the recent year the most exciting development in our opinion was that t
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0067-0057 cesses include: thermonuclear reactions, nebular physics, winds, mass accretion phenomena on compact objects, magnetohydrodynamics, plasmas, thermal and non thermal radiative processes, relativistic phenomena, dust forma­ tion, etc . . In the recent year the most exciting development in our opinion
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0067-0057 resented by the study of variable stars and, in particular, of CV s, as Prof. L. Rosino reminded us at the very beginning of the Congress. We finally chose Aban978-94-010-4148-5978-94-011-0335-0Series ISSN 0067-0057 Series E-ISSN 2214-7985
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