Compact Structure In Active Infrared Dark Cloud Cores

Details Compact Structure In Active Infrared Dark Cloud Cores Compact Structure In Active Infrared Dark Cloud Cores

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop..822b&link_type=abstract

ATNF proposal C1679, Semester: April, 2007

Computer Science

Galactic, Atca

Scientific paper

We will image three active infrared dark cloud cores in HCO+(1-0). We will search for compact protostars and inverse P Cygni profiles that indicate gravitational collapse. These cores were identified as the brightest CS cores in IRDCs mapped with Mopra. Our overall goal is to test the idea that active IRDC cores are in the earliest stages of high-mass protostellar evolution.

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