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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…
Protostars, Dust Globules, and a Herbig-Haro Object in the LMC Superbubble N51D
Y. -H. Chu, R. A. Gruendl, C. -H. R. Chen +9
Using Spitzer Space Telescope and Hubble Space Telescope observations of the superbubble N51D, we have identified three young stellar objects (YSOs) in dust globules, and made the…
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…
The Magnetic Field of the Large Magellanic Cloud: A New Way of Studying Galactic Magnetism
Bryan M. Gaensler, M. Haverkorn, L. Staveley-Smith +4
We present a study of the Faraday rotation of extragalactic sources lying behind the Large Magellanic Cloud. These data represent the most detailed study yet of magnetic field stru…
The magnetic field of the Large Magellanic Cloud revealed through Faraday rotation
B. M. Gaensler, M. Haverkorn, L. Staveley-Smith +4
We have measured the Faraday rotation toward a large sample of polarized radio sources behind the Large Magellanic Cloud (LMC), to determine the structure of this galaxy's magnetic…
A 4.8- and 8.6-GHz Survey of the Large Magellanic Cloud: I The Images
J. R. Dickel, V. J. McIntyre, R. A. Gruendl +1
Detailed 4.8- and 8.6-GHz radio images of the entire Large Magellanic Cloud with half-power beamwidths of 33" at 4.8 GHz and 20" at 8.6 GHz have been obtained using the Australia T…