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An X-ray characterization of the central region of the supernova remnant G332.5-5.6
(Edp Sciences, 2015-10)
Aims. We present an X-ray analysis of the central region of supernova remnant (SNR) G332.5−5.6 through an exhaustive analysis of XMM-Netwon observations with complementary infrared observations. We characterize and discuss ...
A new study of the Supernova Remnant G344.7-0.1 located in the vicinity of the unidentified TeV source HESS J1702-420
(EDP Sciences, 2011-07)
Context. The identification of counterparts of dark gamma-ray sources adds greatly to our understanding of their underlying astrophysical processes. Aims. We investigate the physical properties of the supernova remnant ...
G332.5-5.6, a new Galactic supernova remnant
(Oxford University Press, 2007-12)
We present radio observations of the source G332.5−5.6, a candidate supernova remnant (SNR). Observations have been performed with the Australia Telescope Compact Array (ATCA) at two frequencies, 1.4 and 2.4 GHz. Our results ...
Effects of thermal conduction on the X-ray and synchrotron emission from supernova remnants
(IOP Publishing, 2004-02-01)
Several physical mechanisms have been studied in order to explain why composite supernova remnants (SNRs) have shell-like morphologies in the radio continuum while their X-ray emission is centrally peaked. One of the ...
Proton and Hydrogen Transport through Hydrogen Environments: Ionization and Stripping
(IOP Publishing, 2020-12-23)
Data are presented over a wide range of impact energies describing the ionization or stripping probability, projectile energy loss, and ejected electron and recoiling target energies and angles for proton and hydrogen ...
An X-ray characterization of the central region of the supernova remnant G332.5-5.6
(Edp Sciences, 2015)
XMM-Newton and Chandra observations of G272.2-3.2. Evidence of stellar ejecta in the central region
(Edp Sciences, 2013-03-22)
Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray emitting plasma of the supernova remnant G272.2−3.2 in order to obtain important constraints on its ionization stage, the ...