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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. 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…
X-ray Emission from Wind Blown Bubbles. III. ASCA SIS Observations of NGC6888
M. Wrigge, Y. -H. Chu, E. A. Magnier +1
We present ASCA SIS observations of the wind-blown bubble NGC6888. Owing to the higher sensitivity of the SIS for higher energy photons compared to the ROSAT PSPC, we are able to d…
Parsec-scale X-ray Flows in High-mass Star-forming Regions
L. K. Townsley, P. S. Broos, E. D. Feigelson +1
The Chandra X-ray Observatory is providing remarkable new views of massive star-forming regions, revealing all stages in the life cycle of high-mass stars and their effects on thei…
A Neutral Hydrogen Survey of the Large Magellanic Cloud: Aperture Synthesis and Multibeam Data Combined
S. Kim, L. Staveley-Smith, M. A. Dopita +4
Using a Fourier-plane technique, we have merged HI ATCA and Parkes data sets providing an accurate set of images of the LMC sensitive to structure on scales of 15 pc (for an LMC di…