Supernova remnants interacting with molecular clouds: X-ray and gamma-ray signatures
The giant molecular clouds (MCs) found in the Milky Way and similar galaxies play a crucial
role in the evolution of these systems. The supernova explosions that mark the death of …
role in the evolution of these systems. The supernova explosions that mark the death of …
Detection of the characteristic pion-decay signature in supernova remnants
Cosmic rays are particles (mostly protons) accelerated to relativistic speeds. Despite wide
agreement that supernova remnants (SNRs) are the sources of galactic cosmic rays …
agreement that supernova remnants (SNRs) are the sources of galactic cosmic rays …
Supernova remnants: the X-ray perspective
J Vink - The Astronomy and Astrophysics Review, 2012 - Springer
Supernova remnants are beautiful astronomical objects that are also of high scientific
interest, because they provide insights into supernova explosion mechanisms, and because …
interest, because they provide insights into supernova explosion mechanisms, and because …
Observation of supernova remnant IC 443 with the Fermi large area telescope
We report observation of the supernova remnant (SNR) IC 443 (G189. 1+ 3.0) with the Fermi
Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 …
Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 …
[图书][B] Physics and evolution of supernova remnants
J Vink - 2020 - Springer
When I started working on my PhD project on X-ray spectroscopy of supernova remnants in
1995, one of the things that I missed was a good textbook covering the various aspects of …
1995, one of the things that I missed was a good textbook covering the various aspects of …
Galactic electrons and positrons at the Earth: new estimate of the primary and secondary fluxes
Context. The so-called excess of cosmic ray (CR) positrons observed by the PAMELA
satellite up to 100 GeV has led to many interpretation attempts, from standard astrophysics …
satellite up to 100 GeV has led to many interpretation attempts, from standard astrophysics …
Discriminating the progenitor type of supernova remnants with iron K-shell emission
H Yamaguchi, C Badenes, R Petre… - The Astrophysical …, 2014 - iopscience.iop.org
Supernova remnants (SNRs) retain crucial information about both their parent explosion and
circumstellar material left behind by their progenitor. However, the complexity of the …
circumstellar material left behind by their progenitor. However, the complexity of the …
Search for extended sources in the galactic plane using six years of Fermi-Large Area Telescope pass 8 data above 10 GeV
The spatial extension of a γ-ray source is an essential ingredient to determine its spectral
properties, as well as its potential multiwavelength counterpart. The capability to spatially …
properties, as well as its potential multiwavelength counterpart. The capability to spatially …
Observation of extended very high energy emission from the supernova remnant IC 443 with VERITAS
VA Acciari, E Aliu, T Arlen, T Aune… - The Astrophysical …, 2009 - iopscience.iop.org
We present evidence that the very high energy (VHE, E> 100 GeV) gamma-ray emission
coincident with the supernova remnant IC 443 is extended. IC 443 contains one of the best …
coincident with the supernova remnant IC 443 is extended. IC 443 contains one of the best …
Discovery of strong radiative recombination continua from the supernova remnant IC 443 with Suzaku
H Yamaguchi, M Ozawa, K Koyama… - The Astrophysical …, 2009 - iopscience.iop.org
We present the Suzaku spectroscopic study of the Galactic middle-aged supernova remnant
(SNR) IC 443. The X-ray spectrum in the 1.75–6.0 keV band is described by an optically thin …
(SNR) IC 443. The X-ray spectrum in the 1.75–6.0 keV band is described by an optically thin …