Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-09-08
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
14 pages including 16 figures, to appear in the Astrophysical Journal
Scientific paper
We present a unified model of optical and ultraviolet (UV) light curves for one of the fastest classical novae, V838 Herculis (Nova Herculis 1991), and estimate its white dwarf (WD) mass. Based on an optically thick wind theory of nova outbursts, we model the optical light curves with free-free emission and the UV 1455 \AA light curves with blackbody emission. Our models of 1.35 \pm 0.02 M_\sun WD reproduce simultaneously the optical and UV 1455 \AA observations. The mass lost by the wind is \Delta M_{wind} \sim 2 \times 10^{-6} M_\sun. We provide new determinations of the reddening, E(B-V) = 0.53 \pm 0.05, and of the distance, 2.7 \pm 0.5 kpc.
Cassatella Angelo
Hachisu Izumi
Kato Mariko
No associations
LandOfFree
A Universal Decline Law of Classical Novae. IV. V838 Her (1991): A Very Massive White Dwarf does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Universal Decline Law of Classical Novae. IV. V838 Her (1991): A Very Massive White Dwarf, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Universal Decline Law of Classical Novae. IV. V838 Her (1991): A Very Massive White Dwarf will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-108606