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ABSTRACT 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 1037–1038 erg s−1 at (3.0–3.5) × 105 K or with shocked circumstellar material emitting 1035 erg s−1 by thermal bremsstrahlung at 107 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 (1038 erg s−1) from a
one-solar-mass white dwarf, its effective temperature must be ∼3.5 × 105 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. Access through your institution Buy or subscribe This is a preview of subscription content, access via your institution ACCESS OPTIONS
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16 October 2024 REFERENCES * Ögelman, H., Beuermann, K. & Krautter, J. _Astrophys. J._ 287, L31–L34 (1984). Article ADS Google Scholar * Ögelman, H., Krautter, J. & Beuermann, K.
_Astr. Astrophys._ 177, 110–116 (1987). ADS Google Scholar * Trümper, J. _et al._ _Adv. Space Res._ 2, 241–249 (1983). Article ADS Google Scholar * Greiner, J., Hasinger, G. &
Kahabka, P. _Astr. Astrophys._ 246, L17–L20 (1991). CAS ADS Google Scholar * van den Heuvel, E. P. J., Bhattacharya, D., Nomoto, K. & Rappaport, S. A. _Astr. Astrophys._ 262, 97–105
(1992). CAS ADS Google Scholar * Starrfield, S., Truran, J. W., Sparks, W. M. & Kutter, G. S. _Astrophys. J._ 176, 169–173 (1974). Article ADS Google Scholar * Prialnik, D., Shara,
M. M. & Shaviv, G. _Astr. Astrophys._ 62, 339–348 (1978). CAS ADS Google Scholar * MacDonald, J., Fujimoto, M. Y. & Truran, J. W. _Astrophys. J._ 294, 263–273 (1985). Article
CAS ADS Google Scholar * Starrfield, S., Truran, J. W., Sparks, W. & Krautter, J. in _Extreme Ultraviolet Astronomy_ (eds Malina, R. & Bowyer, S.) 168–176 (Pergamon: New York,
1991). Book Google Scholar * Kato, M. _Publ. Astr. Soc. Japan_ 35, 507–519 (1983). ADS Google Scholar * Orio, M., Trussoni, E. & Ögelman, H. _Astr. Astrophys._ 257, 548–556 (1992).
ADS Google Scholar * Diaz, M. D. & Steiner, J. E. _Astrophys. J._ 239, L41–L43 (1989). Article ADS Google Scholar * Krautter, J. _et al._ _Astr. Astrophys._ 137, 307–326 (1984). CAS
ADS Google Scholar * Diaz, M. P., Williams, R. E., Phillips, M. M. & Steiner, J. E. in _Viña del Mar Workshop on Cataclysmic Variable Stars_ (ed. Vogt, N.) Astr. Soc. Pac. Conf.
Series 29, 362–368 (1992). Google Scholar * Krautter, J. & Williams, R. E. _Astrophys. J._ 341, 968–973 (1989). Article CAS ADS Google Scholar * Orio, M. _et al._ _Proc. 1992 COSPAR
Symp._ (in the press). * Lloyd, H. M. _et al._ _Nature_ 356, 222–224 (1992). Article ADS Google Scholar * Krautter, J., Ögelman, H. & Starrfield, S. _IAU Circ._ no. 5550. * Kovetz,
A., Prialnik, D. & Shara, M. M. _Astrophys. J._ 325, 828–836 (1988). Article ADS Google Scholar * Landau, L. D., Lifshitz, E. M. _The Classical Theory of Fields_, 325 (New York:
Pergamon, 1971). Google Scholar * Verbunt, F. & Zwaan, C. _Astr. Astrophys._ 100, L7–L9 (1981). ADS Google Scholar * Trümper, J. _et al._ _Nature_ 349, 579–583 (1991). Article ADS
Google Scholar * Capaccioli, M., Della Valle, M., D'Onofrio, M. & Rosino, L. _Astrophys. J._ 360, 63–67 (1990). Article ADS Google Scholar * Smale, A. P. _et al._ _Mon. Not. R
astr. Soc._ 233, 51–63 (1988). Article CAS ADS Google Scholar Download references AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * Department of Physics, University of Wisconsin-Madison,
1150 University Avenue, Madison, Wisconsin, 53706, USA Hakki Ögelman * Max-Planck-lnstitut fur Extraterrestrische Physik, D-8046, Garching, Germany Hakki Ögelman * Osservatorio Astronomico
di Torino, 1-10025, Pino Torinese (TO), Italy Marina Orio * Landessternwarte, Konigstuhl, D-6900, Heidelberg, Germany Joachim Krautter * Department of Physics and Astronomy, Arizona State
University, Tempe, Arizona, 85287, USA Sumner Starrfield Authors * Hakki Ögelman View author publications You can also search for this author inPubMed Google Scholar * Marina Orio View
author publications You can also search for this author inPubMed Google Scholar * Joachim Krautter View author publications You can also search for this author inPubMed Google Scholar *
Sumner Starrfield View author publications You can also search for this author inPubMed Google Scholar RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE
Ögelman, H., Orio, M., Krautter, J. _et al._ Detection of supersoft X-ray emission from GQ Muscae nine years after a nova outburst. _Nature_ 361, 331–333 (1993).
https://doi.org/10.1038/361331a0 Download citation * Received: 21 October 1992 * Accepted: 21 December 1992 * Issue Date: 28 January 1993 * DOI: https://doi.org/10.1038/361331a0 SHARE THIS
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