Analysis of the EUVE Survey Observations of Nova Cygni 1992

Details Analysis of the EUVE Survey Observations of Nova Cygni 1992 Analysis of the EUVE Survey Observations of Nova Cygni 1992

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...184.4702m&link_type=abstract

American Astronomical Society, 184th AAS Meeting, #47.02; Bulletin of the American Astronomical Society, Vol. 26, p.937

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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