We report new high-resolution and high-sensitivity radio observations of the extended supernova remnant (SNR) CTB 80 (G69.0+2.7) at 240, 324, 618, and 1380 MHz. The imaging of CTB 80 at 240 and 618 MHz was performed using the Giant Metrewave Radio Telescope in India. The observations at 324 and 1380 MHz were obtained using the Very Large Array of the National Radio Astronomy observatory in its C and D configurations. The new radio images reveal faint extensions for the asymmetric arms of CTB 80. The arms are irregular, with filaments and clumps of size 10 (or 0.6 pc at a distance of 2 kpc). The radio image at 1380 MHz is compared with IR and optical emission. The IR-radio correspondence is excellent along the north arm of CTB 80. Ionized ...
Radio observational results at 232 MHz and multifrequency studies of the supernova remnant (SNR) HB2...
We present new images of the Supernova Remnant (SNR) G127.1+0.5 (R5), based on the 408 MHz and 1420 ...
We describe the serendipitous discovery of a radio point source in a 618-MHz image of the supernova ...
We report new high-resolution and high-sensitivity radio observations of the extended supernova remn...
We report new high-resolution and high-sensitivity radio observations of the extended supernova remn...
We have conducted a study at radio wavelengths of the spectral behaviour of the supernova remnant (S...
(Abridged) We present a detailed radio study of the young supernova remnant (SNR) G292.0+1.8 and its...
We have observed the supernova remnant (SNR) G290.1-0.8 in the 21-cm HI line and the 20-cm radio con...
Aims. We perform a multifrequency radio study of the supernova remnant (SNR) G338.3-0.0, in position...
We present radio-continuum observations of the Galactic supernova remnant (SNR) candidate, G308.3−1....
We present a new millimeter CO-line observation toward supernova remnant (SNR) CTB 87, which was reg...
New images of the radio Supernova Remnant (SNR) G65.1+0.6 are presented, based on the 408 MHz and 14...
Aims. We perform a multifrequency radio study of the supernova remnant (SNR) G338.3−0.0, in position...
We investigated the kinematics of the pulsar wind nebula (PWN) associated with PSR B1951+32 in the o...
New images of the radio Supernova Remnant (SNR) G65.1+0.6 are presented, based on the 408 MHz and 14...
Radio observational results at 232 MHz and multifrequency studies of the supernova remnant (SNR) HB2...
We present new images of the Supernova Remnant (SNR) G127.1+0.5 (R5), based on the 408 MHz and 1420 ...
We describe the serendipitous discovery of a radio point source in a 618-MHz image of the supernova ...
We report new high-resolution and high-sensitivity radio observations of the extended supernova remn...
We report new high-resolution and high-sensitivity radio observations of the extended supernova remn...
We have conducted a study at radio wavelengths of the spectral behaviour of the supernova remnant (S...
(Abridged) We present a detailed radio study of the young supernova remnant (SNR) G292.0+1.8 and its...
We have observed the supernova remnant (SNR) G290.1-0.8 in the 21-cm HI line and the 20-cm radio con...
Aims. We perform a multifrequency radio study of the supernova remnant (SNR) G338.3-0.0, in position...
We present radio-continuum observations of the Galactic supernova remnant (SNR) candidate, G308.3−1....
We present a new millimeter CO-line observation toward supernova remnant (SNR) CTB 87, which was reg...
New images of the radio Supernova Remnant (SNR) G65.1+0.6 are presented, based on the 408 MHz and 14...
Aims. We perform a multifrequency radio study of the supernova remnant (SNR) G338.3−0.0, in position...
We investigated the kinematics of the pulsar wind nebula (PWN) associated with PSR B1951+32 in the o...
New images of the radio Supernova Remnant (SNR) G65.1+0.6 are presented, based on the 408 MHz and 14...
Radio observational results at 232 MHz and multifrequency studies of the supernova remnant (SNR) HB2...
We present new images of the Supernova Remnant (SNR) G127.1+0.5 (R5), based on the 408 MHz and 1420 ...
We describe the serendipitous discovery of a radio point source in a 618-MHz image of the supernova ...