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Session 47 -- Nova Cygni 1992

Display presentation, Wednesday, 1, 1994, 9:20-6:30

[47.02] Analysis of the EUVE Survey Observations of Nova Cygni 1992

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 $T_{eff} \; = \; 3.5 \; 10^{5}$ and $N_{H} \; = \; 2 \; 10^{21}$, 280

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