Joint Astrophysics Colloquium
Joint Astrophysics Seminar
Luminous Infrared Galaxies with the Submillimeter Array:
Probing the Extremes of Star Formation
Christine Wilson
Department of Physics & Astronomy
McMaster University
Luminous and Ultraluminous infrared galaxies (ULIRGs) contain the most
intense regions of star formation in the local universe. Because molecular
gas is the fuel for current and future star formation, the physical
properties and distribution of the warm, dense molecular gas are key
components for understanding the processes and timescales controlling star
formation in these merger and merger remnant galaxies. In this talk, I will
present new results from a legacy project on the Submillimeter Array which
is producing high resolution images of a representative sample of galaxies
with log(L(FIR)) > 11.4 and D < 200 Mpc.
Tuesday, December 4th 2007, 16:00
Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
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