Classical Novae


Classical Novae
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Classical Novae


Classical Novae
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Author : Michael F. Bode
language : en
Publisher: Cambridge University Press
Release Date : 2008-04-07

Classical Novae written by Michael F. Bode and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2008-04-07 with Science categories.


This second edition has been updated and revised and contains contributions covering important developments in this field, and reflecting on interesting insights into classical novae. The book examines thermonuclear processes, the evolution of nova systems, nova atmospheres and winds, the evolution of dust and molecules in novae, nova remnants and observations of novae in other galaxies. It includes observations across the electromagnetic spectrum, from radio to gamma rays, and discusses some of the most important outstanding problems in classical nova research.



Classical Novae


Classical Novae
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Author : Evans Aneurin Bode M F
language : en
Publisher:
Release Date : 2014-05-14

Classical Novae written by Evans Aneurin Bode M F and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2014-05-14 with Science categories.




Physics Of Classical Novae


Physics Of Classical Novae
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Author : International Astronomical Union. Colloquium
language : en
Publisher: Springer
Release Date : 1990

Physics Of Classical Novae written by International Astronomical Union. Colloquium and has been published by Springer this book supported file pdf, txt, epub, kindle and other format this book has been release on 1990 with Science categories.




Classical Novae


Classical Novae
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Author : Michael F. Bode
language : en
Publisher: Cambridge University Press
Release Date : 2012-07-19

Classical Novae written by Michael F. Bode and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-07-19 with Science categories.


This second edition has been updated and revised and contains contributions covering important developments in this field, and reflecting on interesting insights into classical novae. The book examines thermonuclear processes, the evolution of nova systems, nova atmospheres and winds, the evolution of dust and molecules in novae, nova remnants and observations of novae in other galaxies. It includes observations across the electromagnetic spectrum, from radio to gamma rays, and discusses some of the most important outstanding problems in classical nova research.



Classical Nova Explosions


Classical Nova Explosions
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Author : Margarita Hernanz
language : en
Publisher: AIP Conference Proceedings / A
Release Date : 2002-10-31

Classical Nova Explosions written by Margarita Hernanz and has been published by AIP Conference Proceedings / A this book supported file pdf, txt, epub, kindle and other format this book has been release on 2002-10-31 with Medical categories.


The book reviews our current knowledge about Classical Nova Explosions, including all the recent advances from both theoretical and observational points of view. The volume covers a large number of topics, such as the astrophysical scenario, the explosion mechanism (including recent multidimensional approaches), light curves and spectra, and observations based on ground and space facilities, covering all wavelength ranges from radio and infrared to X and gamma-rays. Topics include: novae, cataclysmic variables, nucleosynthesis, white dwarfs, observations (optical, IR, radio, UV, x-rays, gamma-rays).



Classical Novae


Classical Novae
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Author : Michael F. Bode
language : en
Publisher:
Release Date : 1989-05-10

Classical Novae written by Michael F. Bode and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1989-05-10 with Science categories.


A comprehensive, up-to-date description of the properties and mechanisms of classical novae--and the first such effort in the subject since Payne-Gaposchkin's influential (but out of date) The Galactic Novae. Contributors present a balanced mix of observation and theory, and discuss information gathered at optical, radio, infrared, ultraviolet, and x-ray wavelengths. Discussion begins with an overview of the general properties of novae, then covers the accretion process in nova systems and the physics of the nova outburst. Classical novae are then placed in the broader family of cataclysmic variables. Final chapter is devoted to data on novae, including an atlas.



Rs Ophiuchi 1985 And The Recurrent Nova Phenomenon


Rs Ophiuchi 1985 And The Recurrent Nova Phenomenon
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Author : M. F. Bode
language : en
Publisher: VSP
Release Date : 1987-12

Rs Ophiuchi 1985 And The Recurrent Nova Phenomenon written by M. F. Bode and has been published by VSP this book supported file pdf, txt, epub, kindle and other format this book has been release on 1987-12 with Science categories.


This international conference brought together over 50 astronomers from around the world. The meeting centred around a single object, the reccurent nova RS Ophiuchi, a star which had undergone four recorded outbursts before the latest event in 1985. Observations of previous outbursts (discussed in detail in one of the review talks) already indicated that RS Ophiuchi is a unique object of great astronomical significance. The outburst mechanism is probably similar to that of classical novae, but the interaction of the ejecta with a pre-existing shell of material give it the characteristics of a young supernova remnant. However, unlike supernova remnants, the evolution occurs 'before our very eyes'. Following the latest outburst, a frenzy of activity ensued, resulting in the acquisition of detailed observations from the radio (where rapidly expanding jets were discovered) to the X-ray (where RS Ophiuchi turned out to be one of the brightest soft X-ray sources yet observed). The Proceedings report the many exciting and unexpected observational results right across the electromagnetic spectrum in both RS Ophiuchi and related objects. Theoretical work on the cause of the outburst, and remnant evolution is also given prominence. The result is a much fuller understanding of RS Ophiuchi and its important standing in several branches of astrophysical research.



High Sensitivity Radio Astronomy


High Sensitivity Radio Astronomy
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Author : N. Jackson
language : en
Publisher: Cambridge University Press
Release Date : 1997-01-28

High Sensitivity Radio Astronomy written by N. Jackson and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 1997-01-28 with Science categories.


Enhanced sensitivity radio telescopes are producing dramatic results. An international conference was held in Jodrell Bank to take stock of these advances. This timely volume presents the review articles presented by a host of world experts who gathered at this meeting. We are shown how high sensitivity is advancing our understanding in radio spectral line analysis, radio continuum observations of galaxies, cosmology, pulsars, and radio emission from stars; what new and enhanced instruments are now available and those planned for the future. This volume provides graduate students and researchers with an up-to-date and wide-ranging review of the new and future research possible with high-sensitivity radio telescopes.



A Reference Catalogue And Atlas Of Galactic Novae


A Reference Catalogue And Atlas Of Galactic Novae
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Author : Hilmar W. Duerbeck
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-03-09

A Reference Catalogue And Atlas Of Galactic Novae written by Hilmar W. Duerbeck and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-03-09 with Science categories.


4. Census of the Catalogue The catalogue contains information on 277 objects. 137 (50%) of them are stars whose outburst spectra or unambiguous mInImUm characteristics classify them as novae beyond doubt. 123 of them could be identified at minimum. 78 (28 %) are stars with amplitudes and light curve forms which makes nova classifi cation likely. 60 of them could be identified at minimum. Thus, 78 % ofthe objects in this catalogue are confirmed and suspected classical novae. 16 (6%) have properties compatible with both novae and related objects. 15 are identified at minimum. Furthermore, the catalogue and atlas contains data on 12 (4 %) dwarf novae of long cycle length or suspected dwarf novae for which only one outburst has been observed. Examples are WZ Sge and CI Gern. 6 (2%) recurrent novae or suspected recurrent novae are listed. Examples are T CrB and AS Psc. 6 (2%) X-ray novae are listed. Examples are V616 Mon and KY TrA. 6 (2%) symbiotic stars and symbiotic novae are listed. Examples are RT Ser and V352 Aql. 11 (4 %) Mira stars or suspected Mira stars, which at some time were believed to be novae, are listed. Examples are V607 Aql and V927 Sgr.



Novae And Related Stars


Novae And Related Stars
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Author : Yozo Yokota
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06

Novae And Related Stars written by Yozo Yokota and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.


Michael Friedjung Though known since antiquity, novae are still poorly under stood and present many problems. There has tended to be a lack of communication between theoreticians and observers and between different schools of thought, in spite of the advances of recent years in certain directions (observations of ordinary novae at minimum and of dwarf novae, theory of the causes of the explosion, etc ••• ). The meeting whose proceedings are contained in this volume was organized to stimulate a confron tation between the different ideas and results. The subject has changed a lot since 1963, when the previous international meeting was held. There were 61 participants at the conference from 17 countries, so very many groups ~oing research in the field of novae were represented. The reader will see that the subject has become more physical (we know for instance that the binary nature of novae is essential) but much work remains to be done. There is still a large gulf between theory and observation. May he find here many new ideas for future research! I would like to thank the French Centre National de la Recherche Scientifique for providing financial help. I must also thank the other members of the scientific committee (Profs and Drs Bath, Mustel, Payne-Gaposchkin, Sparks and Warner) and of the local committee (Audouze, Mrs Steinberg, Vauclair).