The neon abundance in the ejecta of QU vulpeculae from late-epoch infrared spectra

Robert D. Gehrz, Charles E. Woodward, L. Andrew Helton, Elisha F. Polomski, Thomas L. Hayward, James R. Houck, A. Evans, Joachim Krautter, Steven N. Shore, Sumner Starrfield, James Truran, G. J. Schwarz, R. Mark Wagner

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Abstract

We present ground-based SpectroCam-10 mid-infrared, MMT optical, and Spitzer Space Telescope IRS mid-infrared spectra taken 7.62, 18.75, and 19.38 yr, respectively, after the outburst of the old classical nova QU Vulpeculae (Nova Vul 1984#2). The spectra of the ejecta are dominated by forbidden line emission from neon and oxygen. Our analysis shows that neon was, at the first and last epochs respectively, more than 76 and 168 times overabundant by number with respect to hydrogen compared to the solar value. These high lower limits to the neon abundance confirm that QU VuI involved a thermonuclear runaway on an ONeMg white dwarf, and approach the yields predicted by models of the nucleosynthesis in such events.

Original languageEnglish (US)
Pages (from-to)1167-1173
Number of pages7
JournalAstrophysical Journal
Volume672
Issue number2
DOIs
StatePublished - Jan 10 2008

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Keywords

  • Infrared: stars
  • Novae, cataclysmic variables
  • Stars: individual (QU Vul, Nova Vul 1984 #2)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Gehrz, R. D., Woodward, C. E., Helton, L. A., Polomski, E. F., Hayward, T. L., Houck, J. R., Evans, A., Krautter, J., Shore, S. N., Starrfield, S., Truran, J., Schwarz, G. J., & Wagner, R. M. (2008). The neon abundance in the ejecta of QU vulpeculae from late-epoch infrared spectra. Astrophysical Journal, 672(2), 1167-1173. https://doi.org/10.1086/523660