High Sensitivity XMM X-Ray Observation of R Aquarii

Details High Sensitivity XMM X-Ray Observation of R Aquarii High Sensitivity XMM X-Ray Observation of R Aquarii

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.0305k&link_type=abstract

American Astronomical Society Meeting 210, #03.05; Bulletin of the American Astronomical Society, Vol. 39, p.98

Astronomy and Astrophysics

Astronomy

Scientific paper

A deep observation of R Aquarii in 2005 reveals low surface brightness extended lobe X-ray features not detectable in previous Chandra observations. High sensitivity at 6 keV provides a good quality spectrum of the central source including the Fe fluorescence lines. The RGS spectrum clearly shows the O VII lines in the lobes. Interpretation of these features is presented.

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