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To study the distribution of star formation and dust emission within nearby galaxies, we measured five morphological parameters in the 3.6- and 24-μm wavebands for 65 galaxies in the Spitzer Infrared ...
We present deep and high-resolution Hubble Space Telescope NIC2 F160W imaging at 1.6 μm of six z  2 star-forming galaxies with existing near-infrared integral field spectroscopy from SINFONI at the V...
Supernova remnants (SNRs) are a complex class of sources, and their heterogeneous nature has hindered the characterization of their general observational properties. To overcome this challenge,in thi...
We present initial results from our ongoing program to image the Sunyaev-Zel'dovich (SZ) effect in galaxy clusters at 143 GHz using Bolocam; five clusters and one blank field are described in this man...
Physical mechanisms that shape the morphologies of extragalactic jets。
We present broad band R and narrow band H emission line images of a sample of optically selected starburst galaxies from the Markarian lists. The emission line morphology is studied and global prop...

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