Modeling of the Super-Eddington Phase for Classical Novae: Five IUE Novae
| dc.creator | Kato, Mariko | |
| dc.creator | Hachisu, Izumi | |
| dc.date | 2006-11-18 | |
| dc.date.accessioned | 2026-07-07T10:20:54Z | |
| dc.date.available | 2026-07-07T10:20:54Z | |
| dc.description | 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 Ålight curve, we determine the white dwarf mass and distance to be (1.3 M_sun, 4.4 kpc) for V693 CrA, (1.05 M_sun, 1.8 kpc) for V1974 Cyg, (0.95 M_sun, 4.1 kpc) for V1668 Cyg, (1.0 M_sun, 2.1 kpc) for V351 Pup, and (1.0 M_sun, 4.3 kpc) for OS And. | |
| dc.description | 9 pages including 8 figures, to appear in the Astrophysical Journal | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611594 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611594 | |
| dc.identifier | Astrophys.J.657:1004-1012,2007 | |
| dc.identifier | doi:10.1086/511058 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/174998 | |
| dc.subject | Astrophysics | |
| dc.title | Modeling of the Super-Eddington Phase for Classical Novae: Five IUE Novae | |
| dc.type | text |