Radio continuum study of the Large Magellanic Cloud - SNR J0519-6926

E. J. Crawford; M. D. Filipovic; J. L. Payne

doi:10.2298/SAJ0876059C

Radio continuum study of the Large Magellanic Cloud - SNR J0519-6926

E. J. Crawford, M. D. Filipovic, J. L. Payne

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18 Citations (Scopus)

Abstract

We present the results of new high resolution ATCA observations of SNR J0519-6926. We found that this SNR exhibits a typical "horseshoe" appearance with Î±=0.55ÃƒÂ‚Ã‚Â±0.08 and D=28ÃƒÂ‚Ã‚Â±1 pc. No polarization (or magnetic fields) were detected to a level of 1%. This is probably due to a relatively poor sampling of the UV plane caused be observing in "snap-shot" mode.

Original language	English
Pages (from-to)	59-63
Number of pages	5
Journal	Serbian Astronomical Journal
Volume	176
DOIs	https://doi.org/10.2298/SAJ0876059C
Publication status	Published - 2008

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10.2298/SAJ0876059C

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title = "Radio continuum study of the Large Magellanic Cloud - SNR J0519-6926",

abstract = "We present the results of new high resolution ATCA observations of SNR J0519-6926. We found that this SNR exhibits a typical {"}horseshoe{"} appearance with {\^I}±=0.55{\~A}ƒ{\^A}‚{\~A}‚{\^A}±0.08 and D=28{\~A}ƒ{\^A}‚{\~A}‚{\^A}±1 pc. No polarization (or magnetic fields) were detected to a level of 1%. This is probably due to a relatively poor sampling of the UV plane caused be observing in {"}snap-shot{"} mode.",

author = "Crawford, {E. J.} and Filipovic, {M. D.} and Payne, {J. L.}",

year = "2008",

doi = "10.2298/SAJ0876059C",

language = "English",

volume = "176",

pages = "59--63",

journal = "Serbian Astronomical Journal",

issn = "1450-698X",

publisher = "Astronomical Observatory",

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T1 - Radio continuum study of the Large Magellanic Cloud - SNR J0519-6926

AU - Crawford, E. J.

AU - Filipovic, M. D.

AU - Payne, J. L.

PY - 2008

Y1 - 2008

N2 - We present the results of new high resolution ATCA observations of SNR J0519-6926. We found that this SNR exhibits a typical "horseshoe" appearance with Î±=0.55ÃƒÂ‚Ã‚Â±0.08 and D=28ÃƒÂ‚Ã‚Â±1 pc. No polarization (or magnetic fields) were detected to a level of 1%. This is probably due to a relatively poor sampling of the UV plane caused be observing in "snap-shot" mode.

AB - We present the results of new high resolution ATCA observations of SNR J0519-6926. We found that this SNR exhibits a typical "horseshoe" appearance with Î±=0.55ÃƒÂ‚Ã‚Â±0.08 and D=28ÃƒÂ‚Ã‚Â±1 pc. No polarization (or magnetic fields) were detected to a level of 1%. This is probably due to a relatively poor sampling of the UV plane caused be observing in "snap-shot" mode.

UR - http://handle.uws.edu.au:8081/1959.7/555946

U2 - 10.2298/SAJ0876059C

DO - 10.2298/SAJ0876059C

M3 - Article

SN - 1450-698X

VL - 176

SP - 59

EP - 63

JO - Serbian Astronomical Journal

JF - Serbian Astronomical Journal

ER -

Radio continuum study of the Large Magellanic Cloud - SNR J0519-6926

Abstract

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