Now showing items 1-7 of 7
Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7-3946 with deep H.E.S.S. observations (Corrigendum to article: Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7-3946 with deep HESS observations, 464(1):235-243.)
(EDP Sciences, 2011)
Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7-3946 with deep H.E.S.S. observations (Corrigendum)
Chandra and HESS observations of the supernova remnant CTB 37B
(EDP Sciences, 2008)
We discovered the >100 GeV γ-ray source, HESS J1713−381, apparently associated with the shell-type supernova remnant (SNR) CTB37B, using HESS in 2006. In 2007 we performed X-ray follow-up observations with Chandra with ...
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 ...
A new SNR with TeV shell-type morphology: HESS J1731-347
(EDP Sciences, 2011)
Aims. The recent discovery of the radio shell-type supernova remnant (SNR), G353.6-0.7, in spatial coincidence with the unidentified TeV source HESS J1731−347 has motivated further observations of the source with the High ...
Discovery of gamma-ray emission from the extragalactic pulsar wind nebula N 157B with H.E.S.S
(EDP Sciences, 2012)
We present the significant detection of the first extragalactic pulsar wind nebula (PWN) detected in gamma rays, N 157B, located in the large Magellanic Cloud (LMC). Pulsars with high spin-down luminosity are found to power ...
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 ...
HESS upper limits for Kepler's supernova remnant
(EDP sciences, 2008)
Aims. Observations of Kepler's supernova remnant (G4.5+6.8) with the HESS telescope array in 2004 and 2005 with a total live time of 13 h are presented. Methods. Stereoscopic imaging of Cherenkov radiation from extensive ...