We present results of applying realistic stellar atmosphere models of hot, near Eddington luminosity, high-gravity stars to the EUVE all-sky survey observations of Nova Cygni 1992. Assuming a distance of 2 kpc and envelope composition appropriate for an ONeMg white dwarf, we find Teff ; = ; 3.5 ; 10(5) and NH ; = ; 2 ; 10(21) , 280 days after visual maximum.
American Astronomical Society Meeting Abstracts #184
- Pub Date:
- May 1994