2008ApJ...687.1236H

We present a unified model of infrared (IR), optical, ultraviolet (UV), and X-ray light curves for the 1983 outburst of GQ Muscae (Nova Muscae 1983) and estimate its white dwarf (WD) mass. Based on an optically thick wind model of nova outbursts, we model the optical and IR light curves with free-free emission, and the UV 1455 Å and supersoft X-ray light curves with blackbody emission. The best-fit model that simultaneously reproduces the IR, optical, UV 1455 Å, and supersoft X-ray observations is a 0.7±0.05 M_☉ WD with an assumed chemical composition of the envelope of X=0.35-0.55, X_CNO=0.2-0.35, and Z=0.02 by mass weight. The mass lost by the wind is estimated to be ΔM_wind∼2x10^–5 M_☉. We provide a new determination of the reddening, E(B-V)=0.55±0.05, and of the distance, ∼5 kpc. Finally, we discuss the strong UV flash that took place on JD 2,445,499 (151 days after the outburst).