MIPS Mapping of IC 342 and Maffei 2

Details MIPS Mapping of IC 342 and Maffei 2 MIPS Mapping of IC 342 and Maffei 2

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop50361t&link_type=abstract

Spitzer Proposal ID #50361

Physics

Scientific paper

We propose to map the 24 and 70 micron emission in the disks of the nearby spiral galaxies, IC342 and Maffei 2. These galaxies are among the closest large spirals, actively forming stars, and each showing evidence of recent interaction. MIPS scanning mode is the ideal way to map the star formation, particularly young, obscured star formation, in the outer disks of these close and spatially large galaxies.

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