Aims. Observations of shell-type supernova remnants (SNRs) in the GeV to multi-TeV γ-ray
band, coupled with those at millimetre radio wavelengths, are motivated by the search for …

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 …

Supernova remnants (SNRs) are thought to be the primary sources of Galactic cosmic rays
(CRs). In the last few years, the wealth of γ-ray data collected by GeV and TeV instruments …

The middle-aged supernova remnant (SNR) W44 has recently attracted attention because of
its relevance regarding the origin of Galactic cosmic-rays. For the first time for a SNR, the …

We present the results of GBT observations of all four ground-state hydroxyl (OH) transitions
toward 15 supernova remnants (SNRs) which show OH (1720 MHz) maser emission. This …

Charged particles can be accelerated to high energies by collisionless shock waves in
astrophysical environments, such as supernova remnants. By interacting with the …

We have used the Karl G. Jansky Very Large Array to search for 36 GHz and 44 GHz
methanol (CH 3 OH) lines in a sample of 21 Galactic supernova remnants (SNRs). Mainly …

Very long baseline interferometry, or VLBI, is the observing technique yielding the highest-
resolution images today. Whilst a traditionally large fraction of VLBI observations is …

We present a comprehensive view of the W51B H ii region complex and the W51C
supernova remnant (SNR) using new radio observations from the VLA, VLBA, MERLIN …

Mapping the Dense Molecular Gas toward 13 Supernova Remnants - IOPscience Skip to
content IOP Science home Accessibility Help Search all IOPscience content Search Article …