Nova nucleosynthesis

Sumner Starrfield, J. W. Truran, M. Wiescher, W. M. Sparks

Research output: Contribution to journalArticle

6 Citations (Scopus)

Abstract

We report on the results of hydrodynamic calculations, with updated nuclear reaction rates and opacities, which examine the consequences of the accretion process on 1.25M white dwarfs since that is the most probable mass for the white dwarf in V1974 Cyg 1992.

Original languageEnglish (US)
JournalNuclear Physics A
Volume621
Issue number1-2
StatePublished - Aug 4 1997

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opacity
nuclear fusion
nuclear reactions
reaction kinetics
hydrodynamics

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Starrfield, S., Truran, J. W., Wiescher, M., & Sparks, W. M. (1997). Nova nucleosynthesis. Nuclear Physics A, 621(1-2).

Nova nucleosynthesis. / Starrfield, Sumner; Truran, J. W.; Wiescher, M.; Sparks, W. M.

In: Nuclear Physics A, Vol. 621, No. 1-2, 04.08.1997.

Research output: Contribution to journalArticle

Starrfield, S, Truran, JW, Wiescher, M & Sparks, WM 1997, 'Nova nucleosynthesis', Nuclear Physics A, vol. 621, no. 1-2.
Starrfield S, Truran JW, Wiescher M, Sparks WM. Nova nucleosynthesis. Nuclear Physics A. 1997 Aug 4;621(1-2).
Starrfield, Sumner ; Truran, J. W. ; Wiescher, M. ; Sparks, W. M. / Nova nucleosynthesis. In: Nuclear Physics A. 1997 ; Vol. 621, No. 1-2.
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