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Classical Nova Explosions International Conference on Classical Nova Explosions, Sitges, Spain, 20-24 May, 2002 (AIP Conference Proceedings / Astronomy and Astrophysics) by

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Published by American Institute of Physics .
Written in English

Subjects:

  • Stars, interstellar matter,
  • Stars, New,
  • Medical / Nursing,
  • Astrophysics,
  • Science,
  • Solid State Physics,
  • Science/Mathematics,
  • Physics,
  • Astronomy - Star Guides,
  • General,
  • Science / Astrophysics & Space Science,
  • astrophysical novae,
  • ground-,space-based observations,
  • nova explosion mechanisms,
  • nucliosynthesis,
  • white dwarfs,
  • Astrophysics & Space Science,
  • Congresses

Book details:

Edition Notes

ContributionsMargarita Hernanz (Editor), Jordi Jose (Editor)
The Physical Object
FormatHardcover
Number of Pages590
ID Numbers
Open LibraryOL7889569M
ISBN 10073540092X
ISBN 109780735400924

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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 5/5(1). Buy Classical Novae (Cambridge Astrophysics) on FREE SHIPPING on qualified orders Classical Novae (Cambridge Astrophysics): Michael F. Bode, Aneurin Evans: : Books.   Classical nova captured before, during and after exploding with explosions occurring repeatedly over millions of years. As researchers continue to monitor the binary, they will be looking for. Figure 1: Artist's rendition of a classical nova explosion (Credit: NAOJ) A classical nova explosion is thought to occur on the surface of a white dwarf (center right) with a close companion star.

  Classical novas,such as Nova Centauri , occur in binary star systems, or systems in which two stars orbit around a common center of mass. A white dwarf and another small star orbit a Author: Hanneke Weitering. Classical nova explosions are the third most violent explosions that can occur in a galaxy, exceeded only by a supernova explosion and a γ-ray burst. With total liberated energies of more than 10{su45} erg s{su-1} novae are less energetic than supernovae but nova . Classical nova explosions: International Conference on Classical Nova Explosions: Sitges, Spain, May Classical nova explosions Margarita Hernanz Institut d’Estudis Espacials de Catalunya (CSIC). Campus Universitat Aut`onoma de Barcelona, Facultat de Ci`encies, Torre C5-parell, 2a planta. E Bellaterra (Barcelona), Spain Abstract. A review of the present status of nova modeling is made, with a special emphasis on some specific aspects.