Non-LTE modeling of Nova Cygni 1992

C. Ian Short, Peter H. Hauschildt, Sumner Starrfield, E. Baron

Research output: Contribution to journalArticle

3 Scopus citations

Abstract

We present a grid of nova models that have an extremely large number of species treated in non-LTE and apply it to the analysis of an extensive time series of ultraviolet spectroscopic data for Nova Cygni 1992. We use ultraviolet colors to derive the time development of the effective temperature of the expanding atmosphere during the fireball phase and the first 10 days of the optically thick wind phase. We find that the nova has a pure, optically thick wind spectrum until about 10 days after the explosion. During this interval, we find that synthetic spectra based on our derived temperature sequence agree very well with the observed spectra. We find that a sequence of hydrogen-deficient models provides an equally good fit, provided the model effective temperature is shifted upward by ∼ 1000 K. We find that high-resolution UV spectra of the optically thick wind phase are fit moderately well by the models. We find that a high-resolution spectrum of the fireball phase is better fit by a model with a steep density gradient, similar to that of a supernova, than by a nova model.

Original languageEnglish (US)
Pages (from-to)1057-1070
Number of pages14
JournalAstrophysical Journal
Volume547
Issue number2 PART 1
DOIs
StatePublished - Feb 1 2001

Keywords

  • Novae, cataclysmic variables
  • Stars: atmospheres
  • Stars: individual (Nova Cygni 1992, V1974 Cygni)
  • Ultraviolet: stars

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Non-LTE modeling of Nova Cygni 1992'. Together they form a unique fingerprint.

  • Cite this

    Short, C. I., Hauschildt, P. H., Starrfield, S., & Baron, E. (2001). Non-LTE modeling of Nova Cygni 1992. Astrophysical Journal, 547(2 PART 1), 1057-1070. https://doi.org/10.1086/318413