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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…
XMM-Newton view of the N 206 superbubble in the Large Magellanic Cloud
Patrick J. Kavanagh, Manami Sasaki, Sean. D. Points
We perform an analysis of the X-ray superbubble in the N 206 HII region in the Large Magellanic Cloud using current generation facilities to gain a better understanding of the phys…
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…
The Optical Depth of H II Regions in the Magellanic Clouds
E. W. Pellegrini, M. S. Oey, P. F. Winkler +4
We exploit ionization-parameter mapping as a powerful tool to measure the optical depth of star-forming HII regions. Our simulations using the photoionization code CLOUDY and our n…
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…