The phases of X-ray emission of RS Oph

Jan Uwe Ness, Sumner Starrfield, Kim L. Page, Julian P. Osborne, Andy P. Beardmore, Jeremy J. Drake

Research output: Contribution to journalArticle

1 Scopus citations

Abstract

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.

Original languageEnglish (US)
Pages (from-to)187-190
Number of pages4
JournalProgress of Theoretical Physics Supplement
Issue number169
DOIs
StatePublished - Jan 1 2007

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

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    Ness, J. U., Starrfield, S., Page, K. L., Osborne, J. P., Beardmore, A. P., & Drake, J. J. (2007). The phases of X-ray emission of RS Oph. Progress of Theoretical Physics Supplement, (169), 187-190. https://doi.org/10.1143/PTPS.169.187