The Phases of X-Ray Emission of RS Oph(Chapter 8. White Dwarf and Neutron Star Isolated and/or Binaries, The Extreme Universe in the Suzaku Era)

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概要

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• The recurrent symbiotic nova RS Oph reoccurred after 21 years on 12 February 2006. In contrast to the 1985 outburst, much denser coverage with X-ray observations was achieved. Swift observed RS Oph up to several times a day while Chandra and XMM-Newton observed two to four times during each phase of evolution. While the Swift observations provide high resolution in time, the Chandra and XMM-Newton observations provide high spectral resolution. Refined models can be constrained by the grating spectra, and interpolation of the model parameters can be constrained by the wealth of Swift observations. We compared the Swift light curve with six X-ray observations taken with EXOSAT during the 1985 outburst. We found that the decay from the supersoft X-ray binary (SSS) phase had been observed.

• 2007-12-19

著者

• NESS Jan-Uwe

  School of Earth and Space Exploration, Arizona State University

• Ness Jan-uwe

  School Of Earth And Space Exploration Arizona State University

• Osborne Julian

  Department Of Physics & Astronomy University Of Leicester

• Drake Jeremy

  Harvard-smithsonian Center For Astrophysics

• STARRFIELD Sumner

  School of Earth and Space Exploration, Arizona State University

• PAGE Kim

  Department of Physics & Astronomy, University of Leicester

• BEARDMORE Andy

  Department of Physics & Astronomy, University of Leicester

• Page Kim

  Department Of Physics & Astronomy University Of Leicester

• Beardmore Andy

  Department Of Physics & Astronomy University Of Leicester

• Starrfield Sumner

  School Of Earth And Space Exploration Arizona State University

• Ness Jan‐uwe

  Arizona State Univ. Az Usa

• OSBORNE Julian

  Department of Physics & Astronomy, University of Leicester

• BEARDMORE Andy

  Department of Physics & Astronomy, University of Leicester

• PAGE Kim

  Department of Physics & Astronomy, University of Leicester

関連論文

• X-Ray Spectroscopy of the Classical Nova V458 Vulpeculae with Suzaku
• The Phases of X-Ray Emission of RS Oph(Chapter 8. White Dwarf and Neutron Star Isolated and/or Binaries, The Extreme Universe in the Suzaku Era)
• X-Ray Study of Rekindled Accretion in the Classical Nova V2491 Cygni

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