CHANDRA DETECTION OF EXTENDED X-RAY EMISSION FROM THE RECURRENT NOVA RS OPHIUCHI
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K. Mukai | J. Sokoloski | G. Luna | K. Mukai | J. Kastner | R. Montez | J. H. Kastner | G. J. M. Luna | R. Montez | J. L. Sokoloski | J. Sokoloski | K. Mukai | G. J. M. Luna
[1] Large-Scale Correlations in the Lyα Forest at z = 3-4* , 2004, astro-ph/0405205.
[2] Scott J. Kenyon,et al. An X-ray-emitting blast wave from the recurrent nova RS Ophiuchi , 2006, Nature.
[4] J. P. Osborne,et al. The SSS Phase of RS Ophiuchi Observed with Chandra and XMM-Newton. I. Data and Preliminary Modeling , 2007, 0705.1206.
[5] M. Rupen,et al. An Expanding Shell and Synchrotron Jet in RS Ophiuchi , 2007, 0711.1142.
[6] M. F. Bode,et al. An asymmetric shock wave in the 2006 outburst of the recurrent nova RS Ophiuchi , 2006, Nature.
[7] Marina Orio,et al. X-Ray Spectroscopy of the 2006 Outburst of RS Ophiuchi , 2007, 0709.4512.
[8] Rolf Walder,et al. 3D simulations of RS Ophiuchi : from accretion to nova blast , 2008, 0804.2628.
[9] Michael P. Rupen,et al. Uncovering the Nature of Nova Jets: A Radio Image of Highly Collimated Outflows from RS Ophiuchi , 2008 .
[10] J. Krautter,et al. Swift Observations of the 2006 Outburst of the Recurrent Nova RS Ophiuchi. I. Early X-Ray Emission from the Shocked Ejecta and Red Giant Wind , 2006, astro-ph/0604618.
[11] O. Yaron,et al. An Extended Grid of Nova Models. II. The Parameter Space of Nova Outbursts , 2005 .
[12] P. S. Bunclark,et al. Astronomical Data Analysis Software and Systems , 2008 .
[13] M. T. Schuster,et al. Hubble Space Telescope NICMOS Observations of Classical Nova Shells , 2002 .
[14] Izumi Hachisu,et al. Supersoft X-Ray Light Curve of RS Ophiuchi (2006) , 2007, astro-ph/0703185.
[15] D. Harman,et al. Hubble Space Telescope imaging and ground-based spectroscopy of old nova shells — II. The bipolar shell of the slow nova HR Del , 2003 .
[16] J. Mikolajewska,et al. Spectroscopic orbits and variations of RS Oph , 2009, 0902.2177.
[17] J. Dunlop,et al. A deep optical imaging study of the nebular remnants of classical novae , 1995 .
[18] Gregory Y. Prigozhin,et al. Chandra ACIS Subpixel Event Repositioning: Further Refinements and Comparison between Backside- and Frontside-illuminated X-Ray CCDs , 2004 .
[19] T. J. O'Brien,et al. Hubble Space Telescope imaging and ground-based spectroscopy of old nova shells – I. FH Ser, V533 Her, BT Mon, DK Lac and V476 Cyg , 2000 .
[20] MIT,et al. Outer Jet X-Ray and Radio Emission in R Aquarii: 1999.8 to 2004.0 , 2007, 0705.2570.
[21] J. P. Osborne,et al. Swift X-ray observations of classical novae , 2007 .
[22] E. Serabyn,et al. Interferometric Observations of RS Ophiuchi and the Origin of the Near-Infrared Emission , 2006, astro-ph/0612099.
[23] Gregory Y. Prigozhin,et al. REFINING CHANDRA/ACIS SUBPIXEL EVENT REPOSITIONING USING A BACKSIDE-ILLUMINATED CCD MODEL , 2003 .
[24] M. F. Bode,et al. AMBER/VLTI interferometric observations of the recurrent Nova RS Ophiuchii 5.5 days after outburst , 2006, astro-ph/0611602.
[25] S. Balman,et al. Chandra Observation of the Shell of Nova Persei 1901 (GK Persei): Detection of Localized Nonthermal X-Ray Emission from a Miniature Supernova Remnant , 2005, astro-ph/0503131.
[26] J. J. Drake,et al. Three-dimensional modeling of the asymmetric blast wave from the 2006 outburst of RS Ophiuchi: Early X-ray emission , 2008, 0811.3941.
[27] N. Soker,et al. On the Luminosities and Temperatures of Extended X-Ray Emission from Planetary Nebulae , 2002, astro-ph/0209139.