Aims. We investigate the spatial distribution of the physical and chemical properties of the
hot X-ray emitting plasma of the supernova remnant IC 443, to derive important constraints …

The shocked interstellar medium around IC 443 produces strong X-ray emission in the soft
energy band (E≲ 1.5 keV). We present an analysis of such emission as observed with the …

We present spectral line observations of the ground-state transitions of hydroxyl (OH) toward
supernova remnant (SNR) IC 443 carried out with the Green Bank Telescope. Weak …

Aims. We investigate the morphology at low radio frequencies of the supernova remnant
(SNR) IC 443 in detail and accurately establish its radio continuum spectral properties …

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 …

Context. Supernova remnants (SNRs) represent a major feedback source from stars in the
interstellar medium of galaxies. During the latest stage of supernova explosions, shock …

Context. We study interstellar magnetic fields by measuring the polarization in molecular
spectral lines and thermal emission of dust. Aims. We report detection of non-Zeeman …

We report on a broadband study of a complex X-ray source (1SAX J0618. 0+ 2227)
associated with the interaction site of the supernova remnant (SNR) IC 443 and ambient …

The collisionally pumped, ground-state 1720 MHz maser line of OH is widely recognized as
a tracer for shocked regions and observed in star-forming regions and supernova remnants …

We review the class of galactic supernova remnants which show strong interactions with
molecular clouds, revealed through shock-excited hydroxyl masers. These remnants are …