Composite supernova remnants (SNRs) constitute a small subclass of remnants of massive stellar explosions where non-thermal radiation is observed from both the expanding shell-like shock front and from a pulsar wind nebula (PWN) located inside of the SNR. These systems represent a unique evolutionary phase of SNRs where observations in the radio, X-ray and gamma-ray regimes allow the study of the co-evolution of both of these energetic phenomena. In this article, we report results from observations of the shell-type SNR G15.4+0.1 performed with the High Energy Stereoscopic System (H.E.S.S.) and XMM-Newton. A compact TeV gamma-ray source, HESSJ1818-154, located in the center and contained within the shell of G15.4+0.1 is detected by H.E.S.S....
Supernova remnants exhibit shock fronts (shells) that can accelerate charged particles up to very hi...
The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 ...
A search for new supernova remnants (SNRs) has been conducted using TeV γ-ray data from the H.E.S.S....
Composite supernova remnants (SNRs) constitute a small subclass of remnants of massive stellar explo...
Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar e...
G349.7+0.2 is a young Galactic supernova remnant (SNR) located at the distance of 11.5 kpc and obser...
Aims. Previous observations with the High Energy Stereoscopic System (H.E.S.S.) have revealed an ext...
Young core-collapse supernovae with dense-wind progenitors may be able to accelerate cosmic-ray hadr...
Corrected by: Erratum: H.E.S.S. detection of TeV emission from the interaction region between the su...
The region around the supernova remnant (SNR) W41 contains several TeV sources and has prompted the ...
Aims. Previous observations with the High Energy Stereoscopic System (H.E.S.S.) have revealed an ext...
Supernova remnants exhibit shock fronts (shells) that can accelerate charged particles up to very hi...
The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 ...
A search for new supernova remnants (SNRs) has been conducted using TeV γ-ray data from the H.E.S.S....
Composite supernova remnants (SNRs) constitute a small subclass of remnants of massive stellar explo...
Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar e...
G349.7+0.2 is a young Galactic supernova remnant (SNR) located at the distance of 11.5 kpc and obser...
Aims. Previous observations with the High Energy Stereoscopic System (H.E.S.S.) have revealed an ext...
Young core-collapse supernovae with dense-wind progenitors may be able to accelerate cosmic-ray hadr...
Corrected by: Erratum: H.E.S.S. detection of TeV emission from the interaction region between the su...
The region around the supernova remnant (SNR) W41 contains several TeV sources and has prompted the ...
Aims. Previous observations with the High Energy Stereoscopic System (H.E.S.S.) have revealed an ext...
Supernova remnants exhibit shock fronts (shells) that can accelerate charged particles up to very hi...
The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 ...
A search for new supernova remnants (SNRs) has been conducted using TeV γ-ray data from the H.E.S.S....