The Structure Revealed by Spitzer in NGC 2264

Details The Structure Revealed by Spitzer in NGC 2264 The Structure Revealed by Spitzer in NGC 2264

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pmpa.conf...17t&link_type=abstract

2005: PAST MEETS PRESENT IN ASTRONOMY AND ASTROPHYSICS. Proceedings of the 15th Portuguese National Meeting. Held 28-30 July 200

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present initial results on a very young and highly embedded region of NGC 2264. The 24 μm sources detected are found to be mostly protostellar and spatially located in linear patterns that coincide with dense filaments of molecular material. Furthermore, their quasi-regular separations is consistent with the value for the Jeans length in the region, indicating that the filaments have thernally fragmented and we are observing the primordial substructure of the cluster.

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