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The Fermi Gamma Ray Space Telescope discovers the Pulsar in the Young Galactic Supernova-Remnant CTA 1
Fermi LAT Collaboration
Energetic young pulsars and expanding blast waves (supernova remnants, SNRs) are the most visible remains after massive stars, ending their lives, explode in core-collapse supernov…
OVII and OVIII line emission in the diffuse soft X-ray background: heliospheric and galactic contributions
D. Koutroumpa, F. Acero, R. Lallement +2
We study the 0.57 keV (O VII triplet) and 0.65 keV (O VIII) diffuse emission generated by charge transfer collisions between solar wind (SW) oxygen ions and interstellar H and He n…
The blast wave of Tycho's supernova remnant
Gamil Cassam-Chenai, John P. Hughes, Jean Ballet +1
We use the Chandra X-ray Observatory to study the region in the Tycho supernova remnant between the blast wave and the shocked ejecta interface or contact discontinuity. This zone…
A physical interpretation of the jet-like X-ray emission from supernova remnant W49B
M. Miceli, A. Decourchelle, J. Ballet +4
In the framework of the study of supernova remnants and their complex interaction with the interstellar medium and the circumstellar material, we focus on the galactic supernova re…
The X-ray emission of the supernova remnant W49B observed with XMM-Newton
M. Miceli, A. Decourchelle, J. Ballet +4
In the framework of the study of supernova remnants and their complex interaction with the interstellar medium, we report on an XMM-Newton EPIC observation of the Galactic supernov…
Morphology of synchrotron emission in young supernova remnants
Gamil Cassam-Chenai, Anne Decourchelle, Jean Ballet +1
In the framework of test-particle and cosmic-ray modified hydrodynamics, we calculate synchrotron emission radial profiles in young ejecta-dominated supernova remnants (SNRs) evolv…