141 citations · 261 across the 7 of their papers we have counts for
7 papers
On the influence of shock-cloud interactions on the nonthermal X-ray emission from the supernova remnant RCW 86
Aya Bamba, Hidetoshi Sano, Ryo Yamazaki +1
It is an open issue how the surrounding environment of supernova remnant shocks affect nonthermal X-rays from accelerated electrons, with or without interacting dense material. We…
Detection of optical emission from the supernova remnant G7.7-3.7
V. Domček, J. V. Hernández Santisteban, A. Chiotellis +6
We present the first optical study of the supernova remnant (SNR) G7.7-3.7, with the aim of determining its evolutionary phase since it has been suggested to be the remnant of SN 3…
Detailed spectral and morphological analysis of the shell type SNR RCW 86
H. E. S. S. Collaboration, A. Abramowski, F. Aharonian +232
Aims: We aim for an understanding of the morphological and spectral properties of the supernova remnant RCW~86 and for insights into the production mechanism leading to the RCW~86…
Constraints on cosmic-ray efficiency in the supernova remnant RCW 86 using multi-wavelength observations
M. Lemoine-Goumard, M. Renaud, J. Vink +4
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 nature of this…
Progenitor's signatures in Type Ia supernova remnants
A. Chiotellis, D. Kosenko, K. M. Schure +1
The remnants of Type Ia supernovae can provide important clues about their progenitor-histories. We discuss two well-observed supernova remnants (SNRs) that are believed to result…
The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant
A. Chiotellis, K. M. Schure, Jacco Vink
We present a model for the Type Ia supernova remnant (SNR) of SN 1604, also known as Kepler's SNR. We find that its main features can be explained by a progenitor model of a symbio…
Cosmic-Ray Acceleration Efficiency vs Temperature Equilibration: the Case of SNR 0509-67.5
E. A. Helder, D. Kosenko, J. Vink
We study the 0509-67.5 supernova remnant in the Large Magellanic Cloud with the VLT/FORS2 spectrograph. We detect a broad component in the H-alpha emission with a FWHM of 2680 \pm…