Add to ORKGWe have used the Parkes-MIT-NRAO (PMN) radio survey, at a common frequency of 4.85 GHz (lambda = 6 cm), to study the distribution of Galactic shell supernova remnants (SNRs). We estimate distances and distribution of the Galactic shell SNRs and find the peak of distances to be between 4 and 6 kpc. Our two-dimensional model of the distribution of Galactic shell SNRs shows a concentration between the Sagittarius and the Scutum arms
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
The study of supernova remnants (SNRs) is fundamental to understanding the chemical enrichment and m...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
The Parkes-MIT-NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes-MIT-NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
Supernova remnants (SNRs) in the Galaxy are an important source of energy injection into the interst...
Abstract. The selection effects applicable to the identification of Galactic supernova rem-nants (SN...
We have collected all the available data on Galactic supernova remnants given in the literature. The...
The study of supernova remnants (SNRs) is fundamental to understanding the chemical enrichment and m...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
The study of supernova remnants (SNRs) is fundamental to understanding the chemical enrichment and m...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
The Parkes-MIT-NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes-MIT-NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
The Parkes–MIT–NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic S...
Supernova remnants (SNRs) in the Galaxy are an important source of energy injection into the interst...
Abstract. The selection effects applicable to the identification of Galactic supernova rem-nants (SN...
We have collected all the available data on Galactic supernova remnants given in the literature. The...
The study of supernova remnants (SNRs) is fundamental to understanding the chemical enrichment and m...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...
The study of supernova remnants (SNRs) is fundamental to understanding the chemical enrichment and m...
International audienceThe study of supernova remnants (SNRs) is fundamental to understanding the che...