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Spatially resolved XMM-Newton analysis and a model of the nonthermal emission of MSH 15-52
(EDP Sciences, 2010)
We present an X-ray analysis and a model of the nonthermal emission of the pulsar wind nebula (PWN) MSH 15
−
5
2
. We analyzed
XMM-Newton data to obtain the spatially resolved spectral parameters around the pulsar PSR ...
Numerical simulations of composite supernova remnants for small σ pulsar wind nebulae
(EDP Sciences, 2013)
Context. Composite supernova remnants consist of a pulsar wind nebula located inside a shell-type remnant. The presence of a shell
has implications on the evolution of the nebula, although the converse is generally not ...