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Radio observations of supernova remnants and the surrounding molecular gas
(Societa Astronomica Italiana, 2011-01)
Supernova Remnants (SNRs) are believed to be the main source of Galactic cosmic rays (CR). The strong SNR shocks provide ideal acceleration sites for particles of at least ∼ 1014 eV/nucleon. Radio continuum studies of SNRs ...
Investigation of the Large-scale Neutral Hydrogen near the Supernova Remnant W28
(IOP Publishing, 2002-10)
The distribution and kinematics of neutral hydrogen have been studied in a wide area around the supernova remnant (SNR) W28. A 2fdg5 × 2fdg5 field centered at l = 6fdg5, b = 0° was surveyed using the Parkes 64 m radio ...
An X-ray study of the supernova remnant G20.0-0.2 and its surroundings
(Edp Sciences, 2013-06)
Aims. We study the supernova remnant G20.0-0.2 and its surroundings in order to look for the high energy counterpart of the radio nebula and to find evidence of interaction between the shock front and the interstellar ...
Molecular environments of the supernova remnant G359.1−0.5
(Wiley Blackwell Publishing, Inc, 2020-04)
We report new CO observations and a detailed molecular-line study of the mixed morphology supernova remnant G359.1-0.5, which contains six OH (1720 MHz) masers along the radio shell, indicative of shock-cloud interaction. ...