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Conference Paper: Spectropolarimetry of supernova remnant G296.5 + 10.0
Title | Spectropolarimetry of supernova remnant G296.5 + 10.0 |
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Authors | |
Keywords | Polarization Magnetic fields ISM: supernova remnants ISM: radio continuum X-rays: ISM |
Issue Date | 2008 |
Publisher | Cambridge University Press. |
Citation | International Astronomical Union Symposium S259. In Cosmic Magnetic Fields: From Planets, to Stars and Galaxies-Proceedings of the International Astronomical Union Symposia and Colloquia, 2008, v. 4, p. 141-144 How to Cite? |
Abstract | Radio continuum emission from the supernova remnant G296.5 + 10.0 was observed using the Australia Telescope Compact Array. Using a 104 MHz bandwidth split into 13 × 8 MHz spectral channels, it was possible to produce a pixel-by-pixel image of Rotation Measure (RM) across the entire remnant. A lack of correlation between RM and X-ray surface brightness reveals that the RMs originate from outside the remnant. Using this information, we will characterise the smooth component of the magnetic field within the supernova remnant and attempt to probe the magneto-ionic structure and turbulent scale sizes in the ISM and galactic halo along the line-of-sight. |
Persistent Identifier | http://hdl.handle.net/10722/185543 |
ISBN | |
ISSN | 2023 SCImago Journal Rankings: 0.121 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Harvey-Smith, L | - |
dc.contributor.author | Gaensler, BM | - |
dc.contributor.author | Ng, CY | - |
dc.contributor.author | Green, AJ | - |
dc.date.accessioned | 2013-08-20T07:02:28Z | - |
dc.date.available | 2013-08-20T07:02:28Z | - |
dc.date.issued | 2008 | - |
dc.identifier.citation | International Astronomical Union Symposium S259. In Cosmic Magnetic Fields: From Planets, to Stars and Galaxies-Proceedings of the International Astronomical Union Symposia and Colloquia, 2008, v. 4, p. 141-144 | - |
dc.identifier.isbn | 978-0521889902 | - |
dc.identifier.issn | 1743-9213 | - |
dc.identifier.uri | http://hdl.handle.net/10722/185543 | - |
dc.description.abstract | Radio continuum emission from the supernova remnant G296.5 + 10.0 was observed using the Australia Telescope Compact Array. Using a 104 MHz bandwidth split into 13 × 8 MHz spectral channels, it was possible to produce a pixel-by-pixel image of Rotation Measure (RM) across the entire remnant. A lack of correlation between RM and X-ray surface brightness reveals that the RMs originate from outside the remnant. Using this information, we will characterise the smooth component of the magnetic field within the supernova remnant and attempt to probe the magneto-ionic structure and turbulent scale sizes in the ISM and galactic halo along the line-of-sight. | - |
dc.language | eng | - |
dc.publisher | Cambridge University Press. | - |
dc.relation.ispartof | Cosmic Magnetic Fields: From Planets, to Stars and Galaxies-Proceedings of the International Astronomical Union Symposia and Colloquia | - |
dc.rights | Cosmic Magnetic Fields: From Planets, to Stars and Galaxies-Proceedings of the International Astronomical Union Symposia and Colloquia. Copyright © Cambridge University Press . | - |
dc.subject | Polarization | - |
dc.subject | Magnetic fields | - |
dc.subject | ISM: supernova remnants | - |
dc.subject | ISM: radio continuum | - |
dc.subject | X-rays: ISM | - |
dc.title | Spectropolarimetry of supernova remnant G296.5 + 10.0 | en_US |
dc.type | Conference_Paper | en_US |
dc.identifier.email | Ng, CY: stephen_ng@hku.hk | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1017/S1743921309030373 | - |
dc.identifier.volume | 4 | - |
dc.identifier.spage | 141 | - |
dc.identifier.epage | 144 | - |
dc.identifier.eissn | 1743-9221 | - |
dc.identifier.isi | WOS:000266769600037 | - |
dc.publisher.place | UK | - |
dc.description.other | International Astronomical Union Symposium S259. In Cosmic Magnetic Fields: From Planets, to Stars and Galaxies-Proceedings of the International Astronomical Union Symposia and Colloquia, 2008, v. 4, p. 141-144 | - |
dc.identifier.issnl | 1743-9213 | - |