DETECTION OF SUPERSOFT X-RAY-EMISSION FROM GQ-MUSCAE 9 YEARS AFTER A NOVA OUTBURST

GQ MUS (Nova Muscae 1983) was the first classical nova from which X-rays were detected during outburst1,2. Those Exosat observations were consistent with thermonuclear burning on the surface of a white dwarf emitting 10(37)-10(38) erg s-1 at (3.0-3.5) x 10(5) K or with shocked circumstellar material emitting 10(35) erg s-1 by thermal bremsstrahlung at 10(7) K. Here we report the detection by the Rosat satellite3 of GQ Mus as a very soft black-body-like source. If the observed X-ray flux is being radiated at the Eddington luminosity (10(38) erg s-1) from a one-solar-mass white dwarf, its effective temperature must be approximately 3.5 x 10(5) K. We conclude that the white dwarf is burning hydrogen-rich material near its surface. GQ Mus is, however, the only one of 26 recent novae detected in the all-sky Rosat survey; this suggests that either most novae eject all their accreted material during outburst, or GQ Mus is now burning recently accreted material. GQ Mus appears identical to the supersoft X-ray sources CAL83, CAL87 and RX J0527.8-6954 (ref. 4), lending support to the suggestion that these sources are white dwarfs accreting and burning material from a companion5.