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Conference Paper: Radio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2)

TitleRadio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2)
Authors
Stupar, MiloradFilipovíc, Miroslav D.Jones, Paul A.Parker, Quentin A.
KeywordsISM: individual (RX J0852-4622/G266.2-1.2)
ISM: supernova remnants - radio continuum
Issue Date2005
Citation
Advances in Space Research, 2005, v. 35, n. 6, p. 1047-1051 How to Cite?
DOI: http://dx.doi.org/10.1016/j.asr.2005.02.060
AbstractWe present multi frequency radio-continuum observations of Galactic SNR Vela Z (G266.2-1.2), associated with the prominent X-ray source RX J0852.0-4622 discovered in 1998. Our study of this Galactic supernova remnant (SNR) is based on low-resolution mosaic observations with the ATCA radio interferometer at 1384 and 2496 MHz, Parkes 4850 MHz and MOST 843 MHz survey data. We determine the radio spectral index for the most prominent features of this SNR and compare these features with X-ray observations. We note a sudden spectral turnover at higher then expected frequencies of ∼1384 MHz. © 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/208839
ISSN
0273-1177
2021 Impact Factor: 2.611
2020 SCImago Journal Rankings: 0.682
ISI Accession Number ID
WOS:000231793600012

 

DC FieldValueLanguage
dc.contributor.authorStupar, Milorad-
dc.contributor.authorFilipovíc, Miroslav D.-
dc.contributor.authorJones, Paul A.-
dc.contributor.authorParker, Quentin A.-
dc.date.accessioned2015-03-23T02:01:53Z-
dc.date.available2015-03-23T02:01:53Z-
dc.date.issued2005-
dc.identifier.citationAdvances in Space Research, 2005, v. 35, n. 6, p. 1047-1051-
dc.identifier.issn0273-1177-
dc.identifier.urihttp://hdl.handle.net/10722/208839-
dc.description.abstractWe present multi frequency radio-continuum observations of Galactic SNR Vela Z (G266.2-1.2), associated with the prominent X-ray source RX J0852.0-4622 discovered in 1998. Our study of this Galactic supernova remnant (SNR) is based on low-resolution mosaic observations with the ATCA radio interferometer at 1384 and 2496 MHz, Parkes 4850 MHz and MOST 843 MHz survey data. We determine the radio spectral index for the most prominent features of this SNR and compare these features with X-ray observations. We note a sudden spectral turnover at higher then expected frequencies of ∼1384 MHz. © 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.-
dc.languageeng-
dc.relation.ispartofAdvances in Space Research-
dc.subjectISM: individual (RX J0852-4622/G266.2-1.2)-
dc.subjectISM: supernova remnants - radio continuum-
dc.titleRadio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2)-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1016/j.asr.2005.02.060-
dc.identifier.scopuseid_2-s2.0-21744460726-
dc.identifier.volume35-
dc.identifier.issue6-
dc.identifier.spage1047-
dc.identifier.epage1051-
dc.identifier.isiWOS:000231793600012-
dc.identifier.issnl0273-1177-

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