
Department of Astronomy
You-Hua Chu
Click here for more details.
Professor
Ph.D., University of California, Berkeley, 1981
chu at astro.uiuc.edu
I have been using the Large Magellanic Cloud (LMC) as a laboratory
to study the structuring of the interstellar medium by massive
stars, the subsequent massive star formation triggered by large
interstellar shells, and their implications on galaxy evolution.
The LMC is the only galaxy in which interstellar structures and
their underlying massive stellar population can be studied with
high resolution across the entire galaxy. Studies of
astrophysical processes in the LMC help us understand better our
Milky Way galaxy as well as distant galaxies. The observing
facilities I have used for these studies include Cerro Tololo
Inter-American Observatory, Hubble Space Telescope, ROSAT X-ray
satellite, ASCA X-ray satellite, Chandra X-ray Observatory,
XMM-Newton X-ray satellite, Far-Ultraviolet Spectroscopic
explorer, and Australia Telescope Compact Array.
Selected Recent Publications of Chu: (Click here for a complete list.)
"Supernova Remnants in OB Associations"
Chu, Y.-H.
1997, AJ, 113, 1815.
"ROSAT HRI Survey of the Large Magellanic Cloud"
Chu, Y.-H., and Snowden, S.L.
1998, AN, 319, 101
"Morphology and Physical Structure of the Interstellar Medium"
Chu, Y.-H.
1999, Ap&SS, 269, 441
"A Search for Jovian Planets around Hot White Dwarfs"
Chu, Y.-H., Dunne, B.C., Gruendl, R.A., Brandner, W.
2001, ApJ, 546, L61
"Chandra Reveals the X-ray Glint in the Cat's Eye"
Chu, Y.-H., Guerrero, M.A., Gruendl, R.A., Williams, R.M., Kaler, J.B.
2001, ApJ, 553, L69
Updated: 2001 June 7