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AbstractAbstract
[en] We report on new radio and X-ray observations of two galactic SNRs: G7.7-3.7 and G344.7-0.1. The high resolution, high sensitivity radio data show several new structures in both remnants. In the X-ray regime, the XMM-Newton data for G7.7-3.7 reveal the existence of thermal soft X-ray emission coinciding with the radio southern limb of the remnant, and a point-like feature with a spectrum suggestive of a compact X-ray source or a PWN. In the case of G344.7-0.1, the new XMM-Newton image shows clumpy features and diffuse emission filling the interior of the remnant. The X-ray spectral investigation inferres enhanced abundances which imply the presence of SN ejecta in this SNR.
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International conference on X-ray astronomy 2009: Present status, multi-wavelength approach and future perspectives; Bologna (Italy); 7-11 Sep 2009; (c) 2010 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
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Journal Article
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Conference
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