495 citations · 1.5k across the 31 of their papers we have counts for
31 papers
Peering into the Milky Way by FAST: IV. Identification of two new Galactic supernova remnants G203.1+6.6 and G206.7+5.9
X. Y. Gao, W. Reich, X. H. Sun +5
A 5 7 sky area containing two large radio structures of G203.1+6.6 and G206.7+5.9 with a size of about 2.5 and 3.5 respectively is…
Extended radio halo of the supernova remnant CTB87 (G74.9+1.2)
Wolfgang Reich, Patricia Reich, Roland Kothes
Breaks in the radio spectra of supernova remnants (SNRs) reflect the maximum energy of either shock-accelerated electrons or - in the case of pulsar wind nebulae - of electrons inj…
Radio properties of the optically identified supernova remnant G107.0+9.0
Wolfgang Reich, Xuyang Gao, Patricia Reich
The vast majority of Galactic supernova remnants (SNRs) were detected by their synchrotron radio emission. Recently, the evolved SNR G107.0+9.0 with a diameter of about 3~deg or 75…
New high-frequency radio observations of the Cygnus Loop supernova remnant with the Italian radio telescopes
S. Loru, A. Pellizzoni, E. Egron +19
Supernova remnants (SNRs) represent a powerful laboratory to study the Cosmic-Ray acceleration processes at the shocks, and their relation to the properties of the circumstellar me…
Long, depolarising H-filament towards the Monogem ring
Wolfgang Reich, Patricia Reich, Xiaohui Sun
In soft X-rays, the Monogem ring is an object with a diameter of 25° located in the Galactic anti-centre. It is believed to be a faint, evolved, local supernova remnant. The ring i…
A Radio Continuum and Polarisation Study of the pulsar wind nebula CTB87 (G74.9+1.2)
R. Kothes, W. Reich, S. Safi-Harb +3
We present radio continuum and linear polarisation observations of the pulsar wind nebula CTB87 (G74.9+1.2) with the Effelsberg 100-m radio telescope between 4.75 and 32 GHz. An an…