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Conference Paper: The distance and distribution of galactic supernova remnants from the PMN survey sample

TitleThe distance and distribution of galactic supernova remnants from the PMN survey sample
Authors
Stupar, MFilipovic, MDPannuti, TGParker, QA
Issue Date1-Jan-2004
PublisherAstronomical Society of the Pacific
AbstractWe 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.
Persistent Identifierhttp://hdl.handle.net/10722/341945
ISBN
1-58381-178-8
ISSN
0074-1809
ISI Accession Number ID
WOS:000227426000020

 

DC FieldValueLanguage
dc.contributor.authorStupar, M-
dc.contributor.authorFilipovic, MD-
dc.contributor.authorPannuti, TG-
dc.contributor.authorParker, QA-
dc.date.accessioned2024-03-26T05:38:25Z-
dc.date.available2024-03-26T05:38:25Z-
dc.date.issued2004-01-01-
dc.identifier.isbn1-58381-178-8-
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/10722/341945-
dc.description.abstractWe 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.-
dc.languageeng-
dc.publisherAstronomical Society of the Pacific-
dc.relation.ispartofProceedings of the 195th Symposium of the International Astronomical Union --- Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas-
dc.titleThe distance and distribution of galactic supernova remnants from the PMN survey sample-
dc.typeConference_Paper-
dc.identifier.issue218-
dc.identifier.spage83-
dc.identifier.epage84-
dc.identifier.isiWOS:000227426000020-
dc.publisher.placeSAN FRANCISCO-
dc.identifier.issnl0074-1809-

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