Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3099
Title: A new radio continuum study of the large magellanic cloud supernova remnant MC SNR J0519-6902
Authors: Alsaberi, Rami Z.E.
Filipović, Miroslav D.
Sano, Hidetoshi
Dai, Shi
Haberl, Frank
Kavanagh, Patrick J.
Leahy, Denis
Maggi, Pierre
Rowell, Gavin
Sasaki, Manami
Seitenzahl, Ivo R.
Urošević, Dejan 
Payne, Jeffrey
Smeaton, Zachary J.
Lazarević, Sanja
Affiliations: Astronomy 
Keywords: galaxies: Magellanic Clouds;ISM: supernova remnants;methods: observational
Issue Date: 4-Jun-2025
Rank: M21a
Publisher: Cambridge : Cambridge University Press
Journal: Publications of the Astronomical Society of Australia
Abstract: 
We present a new radio continuum study of the Large Magellanic Cloud supernova remnant (SNR) MC SNR J0519-6902. With a diameter of 8 pc, this SNR shows a radio ring-like morphology with three bright regions towards the north, east, and south. Its linear polarisation is prominent with average values of % and % at 5500 and 9000 MHz, and we find a spectral index of, typical of a young SNR. The average rotation measure is estimated at rad m and the magnetic field strength at G. We also estimate an equipartition magnetic field of G and minimum explosion energy of E = 2.6 erg. Finally, we identified an H i cloud that may be associated with MC SNR J0519-6902, located in the southeastern part of the remnant, along with a potential wind-bubble cavity.
URI: https://research.matf.bg.ac.rs/handle/123456789/3099
ISSN: 13233580
DOI: 10.1017/pasa.2025.10025
Appears in Collections:Research outputs

Show full item record

Google ScholarTM

Check

Altmetric

Altmetric


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.