Protosteller Evolution in the Main Accretion Phase

Details Protosteller Evolution in the Main Accretion Phase Protosteller Evolution in the Main Accretion Phase

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop..286e&link_type=abstract

Spitzer Proposal ID #286

Physics

Scientific paper

I will focus my research on the evolution of the most deeply embedded protostellar objects in their main accretion phase. The projects outlined in my proposal are designed to study the lifetime of the main accretion phase, the innermost envelope structure, the timescale for disk formation, and the disk-to-envelope mass fraction in young protostars. My research will utilize archival Spitzer Legacy data, primarily from the Cores to Disks Legacy Project, as well as proposing new Spitzer IRS and CARMA millimeter interferometric observations of highly embedded protostars.

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