Physics
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.2056k&link_type=abstract
Chandra Proposal ID #07620217
Physics
Chandra Proposal Id #07620217
Scientific paper
We propose to observe a sample of nearby, M82-like, starburst galaxies with high star formation rates. The data will be used to better understand the correlation between the X-ray point population in a galaxy and its star formation rate, to measure the high end of X-ray point source luminosity function to verify or refute the cutoff reported at high luminosities, and, using joint NICMOS and ACS/WFC observations, to study the spatial relation between X-ray source and star forming regions.
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