A prediction of the γ-ray flux from nova herculis 1991

Sumner Starrfield, Steven N. Shore, Warren M. Sparks, George Sonneborn, James W. Truran, Michael Politano

Research output: Contribution to journalArticle

55 Scopus citations

Abstract

Hydrodynamic simulations of thermonuclear runaways in the accreted hydrogen-rich envelopes on 1.0 M, 1.25 M, and 1.35 M white dwarfs predict 22Na and 26Al γ-ray emission from ONeMg novae in outburst. We present and discuss the ultraviolet observations made with the International Ultraviolet Explorer satellite of Nova Her 1991, the most recent bright ONeMg nova. A distance of 3.4 kpc and reddening of E(B-V) = 0.6 to Nova Her 1991 are determined by comparing its UV and optical outburst behavior with those of the extragalactic ONeMg nova LMC 1990 No. 1. Her 1991 was also detected by ROSAT five days into its outburst and we argue that a small fraction of the X-rays may be the product of Comptonized 1.2 and 0.5 MeV emission from the decay of 22Na. If the mass of the ejected shell is indeed as high as has been estimated by Woodward et al., ∼10-4 M, then our results predict that 22Na γ-ray emission from the ejecta of Nova Her 1991 should still be detectable by GRO in the spring of 1992. The detection level is expected to be ∼5 σ in a 2 week observation. Such a detection would strongly guide and constrain the hydrodynamic and nucleosynthesis simulations of nova outbursts on massive white dwarfs.

Original languageEnglish (US)
Pages (from-to)L71-L74
JournalAstrophysical Journal
Volume391
Issue number2 PART 2
DOIs
StatePublished - Jun 1 1992

Keywords

  • Novae, cataclysmic variables
  • Nuclear reactions, nucleosynthesis, abundances

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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