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Spectral Identification of an Ancient Supernova Using Light Echoes in the Large Magellanic Cloud
(2008)
We report the successful identification of the type of the supernova responsible for the supernova remnant SNR 0509-675 in the Large Magellanic Cloud (LMC) using Gemini spectra of surrounding light echoes. The ability to ...
XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
(EDP Sciences, 2004-12)
We present new results from the observations of the supernova remnant (SNR) RX J1713.7–3946 (also G347.3–0.5) performed in five distinct pointings with the EPIC instrument on board the satellite XMM-Newton. RX J1713.7–3946 ...
On the origin of the jet-like radio/X-ray morphology of G290.1-0.8
(EDP Sciences, 2012-10)
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well understood. Several remnants present distorted radio or X-ray shells with jet-like structures. G290.1-0.8 (MSH 11-61A) belongs ...
Mass loss from the progenitor of SN 1006?
(Universidad Nacional Autónoma de México. Instituto de Astronomía, 2008)
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17)
(Edp Sciences, 2010-09-13)
Aims. We report the first detailed X-ray study of the supernova remnant (SNR) G304.6+0.1, achieved with the XMM-Newton mission. Methods. The powerful imaging capability of XMM-Newton was used to study the X-ray characteristics ...
Hard X-ray emission from the SNR G337.2+0.1
(Springer, 2007-06)
We report the hard X-ray emission of the SNR candidate G337.2+0.1. The object shows centrally filled and diffuse X-ray emission, which peaks in the hard 3.0−10.0 keV band. A spectral study confirms that the column density ...
Hard X-ray emission from the SNR G337.2+0.1
(Springer, 2007)