SIMBAD references

2007ApJ...657.1004K - Astrophys. J., 657, 1004-1012 (2007/March-2)

Modeling of the Super-Eddington phase for classical novae: five IUE novae.

KATO M. and HACHISU I.

Abstract (from CDS):

We present a light-curve model for the super-Eddington luminosity phase of five classical novae observed with IUE. Optical and UV light curves are calculated based on the optically thick wind theory with a reduced effective opacity for a porous atmosphere. Fitting a model light curve with the UV 1455 Å light curve, we determine the white dwarf mass and distance to be 1.3 M☉, 4.4 kpc for V693 CrA; 1.05 M☉, 1.8 kpc for V1974 Cyg; 0.95 M☉, 4.1 kpc for V1668 Cyg; 1.0 M☉, 2.1 kpc for V351 Pup; and 1.0 M☉, 4.3 kpc for OS And.

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Journal keyword(s): Stars: Novae, Cataclysmic Variables - stars: individual (OS Andromedae) - stars: individual (V693 Coronae Australis) - Stars: Individual: Constellation Name: V1974 Cygni - stars: individual (V1668 Cygni) - stars: individual (V351 Puppis)

Simbad objects: 6

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