-
Constraints on cosmic-ray efficiency in the supernova remnant RCW 86 using mu...
Several young supernova remnants (SNRs) have recently been detected in the high-energy and very-high-energy gamma-ray domains. As exemplified by RX J1713.7-3946, the... -
Discovery of a Highly Energetic Pulsar Associated with IGR J14003-6326 in the...
We report the discovery of 31.18 ms pulsations from the INTEGRAL source IGR J14003-6326 using the Rossi X-ray Timing Explorer (RXTE). This pulsar is most likely... -
First high-resolution radio study of the supernova remnant G338.3-0.0 associa...
Aims: We perform a multifrequency radio study of the supernova remnant (SNR) G338.3-0.0, in positional coincidence with the TeV source HESS J1640 - 465. We study the... -
Extended Hard X-Ray Emission from the Vela Pulsar Wind Nebula
The nebula powered by the Vela pulsar is one of the best examples of an evolved pulsar wind nebula, allowing access to the particle injection history and the... -
XMM-Newton Observations of MBM 12: More Constraints on the Solar Wind Charge ...
International audience -
FERMI LARGE AREA TELESCOPE DISCOVERY OF GeV GAMMA-RAY EMISSION FROM THE VICIN...
We report the detection of GeV γ-ray emission from the molecular cloud complex that surrounds the supernova remnant (SNR) W44 using the Large Area Telescope on board... -
A Broadband Study of the Emission from the Composite Supernova Remnant MSH 11-62
MSH 11-62 (G291.1-0.9) is a composite supernova remnant for which radio and X-ray observations have identified the remnant shell as well as its central pulsar wind... -
Acceleration of cosmic rays and gamma-ray emission from supernova remnants in...
International audience -
Anisotropic cosmic ray diffusion and gamma-ray production close to supernova ...
International audience
