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Chandra Detection of Extended X-ray Emission from the Recurrent Nova RS Ophiuchi

  • Authors: G. J. M. Luna, R. Montez, J. L. Sokoloski, K. Mukai, and J. H. Kastner

LUNA et al. 2009 The Astrophysical Journal 707 1168.

  • Provider: AAS Journals

Caption: Figure 3.

Images (to which both SER and maximum likelihood deconvolution have been applied) in four energy bands containing roughly the same number of counts (1000). Lower panel: Chandra spectrum of RS Oph (and overlaid best-fit model) with dashed vertical lines indicating the four energy ranges used to generate the four images in the upper panels. The asymmetric X-ray feature is most pronounced in the soft band ( E < 0.77 keV).

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