The thermonuclear runaway and the classical nova outburst

Sumner Starrfield, C. Iliadis, W. R. Hix

Research output: Contribution to journalReview article

33 Citations (Scopus)

Abstract

Nova explosions occur on the white dwarf component of a cataclysmic variable binary stellar system that is accreting matter lost by its companion. When sufficient material has been accreted by the white dwarf, a thermonuclear runaway occurs and ejects material in what is observed as a classical nova explosion. We describe both the recent advances in our understanding of the progress of the outburst and outline some of the puzzles that are still outstanding. We report on the effects of improving both the nuclear reaction rate library and including a modern nuclear reaction network in our one-dimensional, fully implicit, hydrodynamic computer code. In addition, there has been progress in observational studies of supernovae Ia with implications about the progenitors, and we discuss that in this review.

Original languageEnglish (US)
Pages (from-to)1-17
Number of pages17
JournalPublications of the Astronomical Society of the Pacific
Volume128
Issue number963
DOIs
StatePublished - May 1 2016

Fingerprint

nuclear reactions
outburst
explosions
explosion
stellar systems
cataclysmic variables
reaction rate
supernovae
reaction kinetics
hydrodynamics
computer programs
nuclear reaction
material
library
effect
code

Keywords

  • (stars:) novae
  • Cataclysmic variables
  • Stars: evolution
  • Stars: interiors

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

The thermonuclear runaway and the classical nova outburst. / Starrfield, Sumner; Iliadis, C.; Hix, W. R.

In: Publications of the Astronomical Society of the Pacific, Vol. 128, No. 963, 01.05.2016, p. 1-17.

Research output: Contribution to journalReview article

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