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The White Dwarf Mass and the Accretion Rate of Recurrent Novae: an X-ray Perspective
Koji Mukai, Jennifer L. Sokoloski, Thomas Nelson +1
We present recent results of quiescent X-ray observations of recurrent novae (RNe) and related objects. Several RNe are luminous hard X-ray sources in quiescence, consistent with a…
X-ray and UV emission from the recurrent nova RS Ophiuchi in quiescence: Signatures of accretion and shocked gas
Thomas Nelson, Koji Mukai, Marina Orio +2
RS Ophiuchi is a recurrent nova system that experiences outbursts every ~20 years, implying accretion at a high rate onto a massive white dwarf. However, previous X-ray observation…
Detection of X-rays from the symbiotic star V1329 Cyg
Matthias Stute, Gerardo J. M. Luna, Jennifer L. Sokoloski
We report the detection of X-ray emission from the symbiotic star V1329 Cyg with XMM-Newton. The spectrum from the EPIC pn, MOS1 and MOS2 instruments consists of a two-temperature…