Non-thermal X-ray emission from W50 supernova remnant associated with SS433.

Details Non-thermal X-ray emission from W50 supernova remnant associated with SS433. Non-thermal X-ray emission from W50 supernova remnant associated with SS433.

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...19312502s&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #125.02; Bulletin of the American Astronomical Society, Vol. 31, p.669

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the Rossi X-ray Timing Explorer (RXTE) observations of the SNR W50, associated with the jet source SS433. The observations cover the X-ray lobe found between SS433 and the eastern radio `ear' of W50. We combine the X-ray spectrum measured with the Proportional Counter Array (PCA) and the High-Energy Timing Experiment (HEXTE), with the ROSAT and ASCA spectra; thus covering 3 orders of magnitude in energy. We show that the spectrum is well represented by a power law model, and rule out the thermal interpretation of this part of W50. We discuss the non-thermal interpretation in the context of the interaction between the jets from SS433 and the surroundings.

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