139 citations · 890 across the 34 of their papers we have counts for
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Multiwavelength study of the newly confirmed supernova remnant MCSNR J0527-7104 in the Large Magellanic Cloud
Patrick J. Kavanagh, Manami Sasaki, Sean D. Points +6
The Large Magellanic Cloud (LMC) hosts a rich and varied population of supernova remnants (SNRs). Optical, X-ray, and radio observations are required to identify these SNRs, as wel…
Radio-Continuum Observations Of Small, Radially Polarised Supernova Remnant J0519-6902 In The Large Magellanic Cloud
L. M. Bozzetto, M. D. Filipović, D. Urošević +1
We report on new Australian Telescope Compact Array (ATCA) observations of SNR J0519-6902. The Supernova Remnant (SNR) is small in size (~8 pc) and exhibits a typical SNR spectrum…
Multi-frequency study of supernova remnants in the Large Magellanic Cloud. Confirmation of the supernova remnant status of DEM L205
P. Maggi, F. Haberl, L. M. Bozzetto +11
We present new X-ray and radio data of the LMC SNR candidate DEM L205, obtained by XMM-Newton and ATCA, along with archival optical and infrared observations. We use data at variou…
Multi-frequency observations of SNR J0453-6829 in the LMC; A composite supernova remnant with a pulsar wind nebula
F. Haberl, M. D. Filipovic, L. M. Bozzetto +7
The Large Magellanic Cloud (LMC) is rich in supernova remnants (SNRs) which can be investigated in detail with radio, optical and X-ray observations. SNR J0453-6829 is an X-ray and…
Multifrequency radio observations of SNR J0536-6735 (N 59B) with associated pulsar
L. M. Bozzetto, M. D. Filipović, E. J. Crawford +2
We present a study of new Australian Telescope Compact Array (ATCA) observations of supernova remnant, SNR J0536-6735. This remnant appears to follow a shell morphology with a diam…
Multi-Frequency Study of Supernova Remnants in the Large Magellanic Cloud. The case of LMC SNR J0530-7007
A. Y. De Horta, M. D. Filipović, L. M. Bozzetto +12
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 p…
XMMU J0541.8-6659, a new supernova remnant in the Large Magellanic Cloud
M. -H. Grondin, M. Sasaki, F. Haberl +6
The high sensitivity of the XMM-Newton instrumentation offers the opportunity to study faint and extended sources in the Milky Way and nearby galaxies such as the Large Magellanic…