Aims. The Galactic object G78.2+2.1 is a classical shell-type supernova remnant. Previous radio continuum studies have shown substantial variations in spectral index across the object. Existing studies of the neutral hydrogen are of relatively low resolution and sensitivity. Much higher sensitivity and resolution data from the Canadian Galactic Plane Survey justify a re-examination of the properties of this SNR. Methods. In order to improve the accuracy of spectral index determination and its spatial variation, we first remove the underlying thermal emission with the use of a correlation between the $60~\mu$m infrared continuum and 1420 MHz radio continuum. We use the so-called TT-plot technique to obtain the continuum spectral inde...
Abstract: G192.81.1 has been known as one of the faintest supernova remnants (SNRs) in the Galaxy un...
Context. More than 90% of the known Milky Way supernova remnants (SNRs) are within 5\ub0 of the Gala...
Supernovae and supernova remnants are salient astrophysical sources for their importance in nucleosy...
We report on observations of the candidate supernova remnant (SNR) G106.3+2.7 with the Dominion Radi...
Aims. The supernova remnant (SNR) G15.4+0.1 is considered to be the possible counterpart of the γ-ra...
We present new images of the Supernova Remnant (SNR) G127.1+0.5 (R5), based on the 408 MHz and 1420 ...
The distribution and kinematics of neutral hydrogen have been studied in a wide area around the supe...
Although the Galactic supernova remnant (SNR) G46.8–0.3 has been known for more than 50 yr, no speci...
We have identified a new supernova remnant (SNR), G51.04+0.07, using observations at 74 MHz from the...
We present new images of the low radio surface brightness Supernova Remnant (SNR) G126.2+1.6, based ...
New images of the radio Supernova Remnant (SNR) G65.1+0.6 are presented, based on the 408 MHz and 14...
International audienceContext. The properties of the population of Galactic supernova remnants (SNRs...
grantor: University of TorontoYoung, massive stars profoundly affect the interstellar medi...
We present compelling evidence for confirmation of a Galactic supernova remnant (SNR) candidate, G33...
Context. While over 1000 supernova remnants (SNRs) are estimated to exist in the Milky Way, only les...
Abstract: G192.81.1 has been known as one of the faintest supernova remnants (SNRs) in the Galaxy un...
Context. More than 90% of the known Milky Way supernova remnants (SNRs) are within 5\ub0 of the Gala...
Supernovae and supernova remnants are salient astrophysical sources for their importance in nucleosy...
We report on observations of the candidate supernova remnant (SNR) G106.3+2.7 with the Dominion Radi...
Aims. The supernova remnant (SNR) G15.4+0.1 is considered to be the possible counterpart of the γ-ra...
We present new images of the Supernova Remnant (SNR) G127.1+0.5 (R5), based on the 408 MHz and 1420 ...
The distribution and kinematics of neutral hydrogen have been studied in a wide area around the supe...
Although the Galactic supernova remnant (SNR) G46.8–0.3 has been known for more than 50 yr, no speci...
We have identified a new supernova remnant (SNR), G51.04+0.07, using observations at 74 MHz from the...
We present new images of the low radio surface brightness Supernova Remnant (SNR) G126.2+1.6, based ...
New images of the radio Supernova Remnant (SNR) G65.1+0.6 are presented, based on the 408 MHz and 14...
International audienceContext. The properties of the population of Galactic supernova remnants (SNRs...
grantor: University of TorontoYoung, massive stars profoundly affect the interstellar medi...
We present compelling evidence for confirmation of a Galactic supernova remnant (SNR) candidate, G33...
Context. While over 1000 supernova remnants (SNRs) are estimated to exist in the Milky Way, only les...
Abstract: G192.81.1 has been known as one of the faintest supernova remnants (SNRs) in the Galaxy un...
Context. More than 90% of the known Milky Way supernova remnants (SNRs) are within 5\ub0 of the Gala...
Supernovae and supernova remnants are salient astrophysical sources for their importance in nucleosy...