To uniformly determine the properties of supernova remnants (SNRs) at high energies, we
have developed the first systematic survey at energies from 1 to 100 GeV using data from …

Aims. We study the spectral and polarization properties of supernova remnants (SNRs)
using our λ6 cm survey data. Methods. We analyse data from observations taken as part of …

We carry out a project to independently measure the distances of supernova remnants
(SNRs) in the first quadrant of the Galaxy. In this project, red clump (RC) stars are used as …

As part of a systematic search programme of a 10° wide strip of the northern Galactic plane,
we present preliminary evidence for the discovery of four (and possibly five) new supernova …

We present optical CCD images of the large supernova remnant (SNR) G 132.7+ 1.3 (HB3)
covering its full extent for the first time, in the emission lines of Hα+[N ii],[S ii], and [O iii] …

Context. About 15%-60% of all supernova remnants are estimated to interact with dense
molecular clouds. In these high-density environments, radiative losses are significant. The …

Abstract We present full Stokes MeerKAT L-band (856–1712 MHz) observations of 36 high-
latitude supernova remnants (SNRs). Sensitive, high-dynamic-range images show a wealth …

During detailed searches for new Galactic supernova remnants (SNRs) in the Anglo-
Australian Observatory/United Kingdom Schmidt Telescope (AAO/UKST) Hα survey of the …

Deep optical CCD images of the supernova remnant G 32.8-0.1 were obtained where
filamentary and diffuse emission was discovered. The images were acquired in the emission …

The supernova remnant (SNR) candidate G 116.6− 26.1 is one of the few high Galactic
latitude (| b|> 15°) remnants detected so far in several wavebands. It was discovered …