Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop..249i&link_type=abstract
Spitzer Proposal ID #249
Physics
Scientific paper
Massive stars dominate the energetics and evolution of the visible universe through their ionizing radiation, winds, and supernova explosions. Despite significant recent progress in understanding low-mass star formation, high-mass star formation is still a mystery. I will survey star forming regions in the inner and outer Galaxy and the LMC, to discover the obscured stellar content, analyze the proto-cluster and protostellar luminosity function, and probe the radiation and gas physics in star forming regions. The resolution and sensitivity of Spitzer is allowing, for the first time, a relatively unconfused analysis of star forming regions in extremely diverse environments.
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