Star formation in Perseus. II. (Hatchell+, 2007)

Details Star formation in Perseus. II. (Hatchell+, 2007) Star formation in Perseus. II. (Hatchell+, 2007)

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34681009h&link_type=abstract

VizieR On-line Data Catalog: J/A+A/468/1009. Originally published in: 2007A&A...468.1009H

Computer Science

Scientific paper

We compile spectral energy distributions (SEDs) from 2MASS (1-2um), Spitzer IRAC (3.6, 4.5, 5.8, 8.0um), Michelle (11 and 18um), IRAS (12, 25, 60, 100um), SCUBA (450 and 850um) and Bolocam (1100um) data. Sources are classified starless/protostellar on the basis of infrared and/or outflow detections and Class I/Class 0 on the basis of Tbol, Lbol/Lsmm and F3.6/F850. In order to investigate the dependence of these evolutionary indicators on mass, we construct radiative transfer models of Class 0 sources.
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