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- Publisher Website: 10.1016/j.asr.2005.02.060
- Scopus: eid_2-s2.0-21744460726
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Conference Paper: Radio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2)
Title | Radio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2) |
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Authors | |
Keywords | ISM: individual (RX J0852-4622/G266.2-1.2) ISM: supernova remnants - radio continuum |
Issue Date | 2005 |
Citation | Advances in Space Research, 2005, v. 35, n. 6, p. 1047-1051 How to Cite? |
Abstract | We 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 Identifier | http://hdl.handle.net/10722/208839 |
ISSN | 2023 Impact Factor: 2.8 2023 SCImago Journal Rankings: 0.663 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Stupar, Milorad | - |
dc.contributor.author | Filipovíc, Miroslav D. | - |
dc.contributor.author | Jones, Paul A. | - |
dc.contributor.author | Parker, Quentin A. | - |
dc.date.accessioned | 2015-03-23T02:01:53Z | - |
dc.date.available | 2015-03-23T02:01:53Z | - |
dc.date.issued | 2005 | - |
dc.identifier.citation | Advances in Space Research, 2005, v. 35, n. 6, p. 1047-1051 | - |
dc.identifier.issn | 0273-1177 | - |
dc.identifier.uri | http://hdl.handle.net/10722/208839 | - |
dc.description.abstract | We 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.language | eng | - |
dc.relation.ispartof | Advances in Space Research | - |
dc.subject | ISM: individual (RX J0852-4622/G266.2-1.2) | - |
dc.subject | ISM: supernova remnants - radio continuum | - |
dc.title | Radio continuum observations of the galactic supernova remnant Vela Z (G266.2-1.2) | - |
dc.type | Conference_Paper | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1016/j.asr.2005.02.060 | - |
dc.identifier.scopus | eid_2-s2.0-21744460726 | - |
dc.identifier.volume | 35 | - |
dc.identifier.issue | 6 | - |
dc.identifier.spage | 1047 | - |
dc.identifier.epage | 1051 | - |
dc.identifier.isi | WOS:000231793600012 | - |
dc.identifier.issnl | 0273-1177 | - |