The Supersoft X-ray Phase of Nova RS Ophiuchi 2006

Swift X-ray observations of the ~60 day supersoft phase of the recurrent nova RS Ophiuchi (RS Oph) 2006 show the progress of nuclear burning on the white dwarf (WD) in exquisite detail. First seen 26 days after the optical outburst, this phase started with extreme variability likely due to variable...

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Veröffentlicht in:	The Astrophysical journal 2011-02, Vol.727 (2), p.124-jQuery1323911611911='48'
Hauptverfasser:	Osborne, J. P, Page, K. L, Beardmore, A. P, Bode, M. F, Goad, M. R, O'Brien, T. J, Starrfield, S, Rauch, T, Ness, J.-U, Krautter, J, Schwarz, G, Burrows, D. N, Gehrels, N, Drake, J. J, Evans, A, Eyres, S. P. S
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BINARY STARS Combustion DWARF STARS ELECTROMAGNETIC RADIATION ERUPTIVE VARIABLE STARS IONIZING RADIATIONS Luminosity Nova NOVAE OSCILLATIONS Outbursts RADIATIONS Signatures SOFT X RADIATION STARS Supernovas Temperature VARIABLE STARS WHITE DWARF STARS X RADIATION X-rays
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