Skip to content
Home
About Us
Resources
Profiles Metrics
Authors Directory
Institutions Directory
Top Authors
Top Institutions
Top Sponsors
AI Digest
Contact Us
Menu
Home
About Us
Resources
Profiles Metrics
Authors Directory
Institutions Directory
Top Authors
Top Institutions
Top Sponsors
AI Digest
Contact Us
Home
About Us
Resources
Profiles Metrics
Authors Directory
Institutions Directory
Top Authors
Top Institutions
Top Sponsors
AI Digest
Contact Us
Menu
Home
About Us
Resources
Profiles Metrics
Authors Directory
Institutions Directory
Top Authors
Top Institutions
Top Sponsors
AI Digest
Contact Us
Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
earth and planetary sciences
Multi-frequency study of supernova remnants in the Large Magellanic Cloud: The case of LMC SNR J0530-7007
Astronomy and Astrophysics, Volume 540, Article A25, Year 2012
Notification
URL copied to clipboard!
Description
Context. The supernova remnants (SNRs) known in the Large Magellanic Cloud (LMC) show a variety of morphological structures in the different wavelength bands. This variety is the product of the conditions in the surrounding medium with which the remnant interacts and the inherent circumstances of the supernova event itself. Aims. This paper performs a multi-frequency study of the LMC SNR J0530-7007 by combining Australia Telescope Compact Array (ATCA), Molonglo Observatory Synthesis Telescope (MOST), Röntgensatellit (ROSAT) and Magellanic Clouds Emission Line Survey (MCELS) observations. Methods. We analysed radio-continuum, X-ray and optical data and present a multi-wavelength morphological study of LMC SNR J0530-7007. Results. We find that this object has a shell-type morphology with a size of 215′′ × 180′′ (52 pc × 44 pc); a radio spectral index (α =-0.85 ± 0.13); with [S II]/Hα > 0.4 in the optical; and the presence of non-thermal radio and X-ray emission. Conclusions. We confirmed this object as a bona-fide shell-type SNR which is probably a result of a Type Ia supernova. © 2012 ESO.
Authors & Co-Authors
de Horta, Ain Y.
Australia, Penrith
Western Sydney University
Filipovíc, Miroslav D.
Australia, Penrith
Western Sydney University
Bozzetto, Luke M.
Australia, Penrith
Western Sydney University
Maggi, Pierre
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Haberl, Frank W.
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Crawford, Evan J.
Australia, Penrith
Western Sydney University
Sasaki, Manami
Germany, Tubingen
Eberhard Karls Universität Tübingen
Urošević, Dejan
Serbia, Belgrade
University of Belgrade
Serbia, Belgrade
Isaac Newton Institute of Chile
Pietsch, Wolfgang N.
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Gruendl, Robert A.
United States, Urbana
University of Illinois Urbana-champaign
Dickel, John R.
United States, Albuquerque
The University of new Mexico
Tothill, Nicholas F.H.
Australia, Penrith
Western Sydney University
Chu, Youhua
United States, Urbana
University of Illinois Urbana-champaign
Payne, Jeffrey L.
Australia, Penrith
Western Sydney University
Collier, Jordan D.
Australia, Penrith
Western Sydney University
Statistics
Citations: 23
Authors: 15
Affiliations: 7
Identifiers
Doi:
10.1051/0004-6361/201118694
ISSN:
00046361
Research Areas
Environmental
Study Design
Cross Sectional Study
Study Approach
Quantitative