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The Suzaku Observations of SS Cygni in Quiescence and Outburst
Manabu Ishida, Shunsaku Okada, Takayuki Hayashi +4
We present results from the Suzaku observations of the dwarf nova SS Cyg in quiescence and outburst in 2005 November. Owing to high sensitivity of the HXD PIN detector and high spe…
RS Ophiuchi in Quiescence: Why is it X-ray Faint?
Koji Mukai
The short interval between successive outbursts of RS Oph strongly suggests that it has a high mass white dwarf accreting at a high rate. This, in turn, suggests the possibility of…
High energy X-ray emission from recurrent novae in quiescence: T CrB
Gerardo J. M. Luna, Jennifer L. Sokoloski, Koji Mukai
We present Suzaku X-ray observations of the recurrent nova T CrB in quiescence. T CrB is the first recurrent nova to be detected in the hard-X-ray band (E ~ 40.0 keV) during quiesc…
XMM-Newton Observations of the Cataclysmic Variable GW Lib
Eric J. Hilton, Paula Szkody, Anjum Mukadam +4
XMM-Newton observations of the accreting, pulsating white dwarf in the quiescent dwarf nova GW Librae were conducted to determine if the non-radial pulsations present in previous U…
Recent Advances in X-ray Observations of Cataclysmic Variables
K. Mukai
A personal selection of noteworthy X-ray results on CVs are presented, with emphasis on XMM-Newton and Chandra observations. Progressing roughly from broad-band view to narrow-band…
A Chandra LETGS observation of V4743 Sagittarius: A Super Soft X-ray Source and a Violently Variable Light Curve
J. -U. Ness, S. Starrfield, V. Burwitz +13
V4743 Sgr (Nova Sgr 2002 No. 3) was discovered on 20 September 2002. We obtained a 5ks ACIS-S spectrum in November 2002 and found that the nova was faint in X-rays. We then obtaine…