40 citations · 71 across the 3 of their papers we have counts for
6 papers
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 […
Star Formation in the LMC: Gravitational Instability and Dynamical Triggering
Y. -H. Chu, R. A. Gruendl, C. -C. Yang
Evidence for triggered star formation is difficult to establish because energy feedback from massive stars tend to erase the interstellar conditions that led to the star formation.…
Supernova Remnants in the Magellanic Clouds. VII. Infrared Emission from SNRs
R. M. Williams, Y. -H. Chu, R. Gruendl
We have used the instruments on the Spitzer Space Telescope to study the Large Magellanic Cloud supernova remnants (SNRs) N11L, N44, N49, N206, N63A, and N157B. The two large SNRs…
An Optical Study of Stellar and Interstellar Environments of Seven Luminous and Ultraluminous X-Ray Sources
Caitlin J. Ramsey, Rosa M. Williams, Robert A. Gruendl +3
We have studied the stellar and interstellar environments of two luminous X-ray sources and five ultraluminous X-ray sources (ULXs) in order to gain insight into their nature. Arch…
Supernova Remnants in the Magellanic Clouds. IV. X-Ray Emission from the Largest SNR in the LMC
R. M. Williams, Y. -H. Chu, J. R. Dickel +4
We present the first X-ray detection of SNR 0450-70.9 the largest known supernova remnant (SNR) in the Large Magellanic Cloud. To study the physical conditions of this SNR, we have…
XMM-Newton observations of the giant HII region N11 in the LMC
Y. Naze, I. I. Antokhin, G. Rauw +2
Using the sensitive XMM-Newton observatory, we have observed the giant HII region N11 in the LMC for \sim30 ks. We have detected several large areas of soft diffuse X-ray emission…