Distributed vs. Clustered Star Formation in Mon OB1 - NGC 2264

Details Distributed vs. Clustered Star Formation in Mon OB1 - NGC 2264 Distributed vs. Clustered Star Formation in Mon OB1 - NGC 2264

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40006f&link_type=abstract

Spitzer Proposal ID #40006

Physics

Scientific paper

Following successful IRAC + MIPS observations (75% complete) of the GMCs Cep OB3 and Mon R2 harboring high mass star formation in PID 20403 'Distributed vs. Clustered Star Formation', we propose in this cycle to obtain similar observations for 2 more GMCs, namely Mon OB1 and Cam OB1. The present GTO proposal begins this program by covering part of the distributed area around NGC 2264 in Mon OB1. The rest of Mon OB1 as well as Cam OB1 will be proposed as a GO program. We hope to establish the physical conditions leading to clustered vs. distributed star formation. We will compare results for all these regions against similar studies in clouds harboring low mass star formation, for example, the c2d survey.

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