File Download

There are no files associated with this item.

Supplementary

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, QAGaensler, BM
Editors
Editor(s):Camilo, F
Issue Date2003
PublisherAstronomical Society of the Pacific
Citation
Young Neutron Stars and Their Environments, IAU Symposium no. 218, Sydney, Australia, 14-17 July 2003, p. 83-83 How to Cite?
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/10722/211259

 

DC FieldValueLanguage
dc.contributor.authorStupar, M-
dc.contributor.authorFilipovic, MD-
dc.contributor.authorPannuti, TG-
dc.contributor.authorParker, QA-
dc.contributor.authorGaensler, BM-
dc.contributor.editorCamilo, F-
dc.date.accessioned2015-07-08T03:23:49Z-
dc.date.available2015-07-08T03:23:49Z-
dc.date.issued2003-
dc.identifier.citationYoung Neutron Stars and Their Environments, IAU Symposium no. 218, Sydney, Australia, 14-17 July 2003, p. 83-83-
dc.identifier.urihttp://hdl.handle.net/10722/211259-
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.ispartofYoung Neutron Stars and Their Environments-
dc.titleThe Distance and Distribution of Galactic Supernova Remnants from the PMN Survey Sample-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.volume218-
dc.identifier.spage83-
dc.identifier.epage83-
dc.publisher.placeSan Francisco, CA-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats