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HIGH-RESOLUTION X-RAY SPECTROSCOPY OF THE GALACTIC SUPERNOVA REMNANT PUPPIS A WITH XMM-NEWTON /RGS
We present high-resolution X-ray spectra of cloud-shock interaction regions in the eastern and northern rims of the Galactic supernova remnant Puppis A, using the Reflection Grating Spectrometer on board the XMM-Newton satellite. A number of emission lines including K[alpha] triplets of He-like N, O...
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Published in: | The Astrophysical journal 2012-09, Vol.756 (1), p.1-7 |
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container_title | The Astrophysical journal |
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creator | Katsuda, Satoru Tsunemi, Hiroshi Mori, Koji Uchida, Hiroyuki Petre, Robert Yamada, Shin'ya Akamatsu, Hiroki KONAMI, SAORI Tamagawa, Toru |
description | We present high-resolution X-ray spectra of cloud-shock interaction regions in the eastern and northern rims of the Galactic supernova remnant Puppis A, using the Reflection Grating Spectrometer on board the XMM-Newton satellite. A number of emission lines including K[alpha] triplets of He-like N, O, and Ne are clearly resolved for the first time. Intensity ratios of forbidden to resonance lines in the triplets are found to be higher than predictions by thermal emission models having plausible plasma parameters. The anomalous line ratios cannot be reproduced by effects of resonance scattering, recombination, or inner-shell ionization processes, but could be explained by charge-exchange emission that should arise at interfaces between the cold/warm clouds and the hot plasma. Our observations thus provide observational support for charge-exchange X-ray emission in supernova remnants. |
doi_str_mv | 10.1088/0004-637X/756/1/49 |
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subjects | Clouds Emission Ionization Mathematical models Spectrometers Supernova remnants X-rays XMM (spacecraft) |
title | HIGH-RESOLUTION X-RAY SPECTROSCOPY OF THE GALACTIC SUPERNOVA REMNANT PUPPIS A WITH XMM-NEWTON /RGS |
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