Cluster Evolution In The Rosette Molecular Cloud Main Core Region

Details Cluster Evolution In The Rosette Molecular Cloud Main Core Region Cluster Evolution In The Rosette Molecular Cloud Main Core Region

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21813009y&link_type=abstract

American Astronomical Society, AAS Meeting #218, #130.09; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Using Spitzer Space Telescope and Chandra X-ray data, we identify YSOs in the RMC main core region. Nearest Neighbor Method (NNM) was employed to analyze the structures and distributions of Class I/0, Class II, and Class III sources. Additionally, we developed a ratio mapping technique to investigate the progression of star formation. We discuss the distribution of YSOs, progression of star formation, and structure of the clusters in this region.
This work is based in part on archival data obtained with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by an award issued by JPL/Caltech, Florida Space Grant Consortium, and a NASA GSRP fellowship.

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