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Supernova Remnants in the Large Magellanic Clouds IX: Multiwavelength Analysis of the Physical Structure of N49
J. Bilikova, R. N. M. Williams, Y. -H. Chu +2
We present a multiwavelength analysis of the supernova remnant N49 in the Large Magellanic Cloud. Using high-resolution Hubble Space Telescope WFPC2 images of H-alpha, [S II] and […
Chandra Observation of the Magellanic Cloud Supernova Remnant 0454-672 in N9
F. D. Seward, R. M. Williams, Y. -H. Chu +3
A Chandra observation has defined the extent of the SNR B 0454-692 in the LMC H II region N9. The remnant has dimension 2.3" x 3.6" and is elongated in the NS direction. The bright…
Supernova Remnants in the Magellanic Clouds. VI. The DEML316 Supernova Remnants
R. M. Williams, Y. -H. Chu
The DEML316 system contains two shells, both with the characteristic signatures of supernova remnants (SNRs). We analyze Chandra and XMM-Newton data for DEML316, investigating its…
Supernova Remnants in the Magellanic Clouds. V. The Complex Interior Structure of the N206 SNR
R. M. Williams, Y. -H. Chu, J. R. Dickel +4
The N206 supernova remnant (SNR) in the Large Magellanic Cloud (LMC) has long been considered a prototypical "mixed morphology" SNR. Recent observations, however, have added a new…