Star Formation Studies with ALMA in Cycle 0 and Cycle 1

Details Star Formation Studies with ALMA in Cycle 0 and Cycle 1 Star Formation Studies with ALMA in Cycle 0 and Cycle 1

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21930903s&link_type=abstract

American Astronomical Society, AAS Meeting #219, #309.03

Astronomy and Astrophysics

Astronomy

Scientific paper

In the next few years, ALMA observations of dense cores will revolutionize our understanding of star formation. In this talk, I shall highlight the capabilities of ALMA in Cycle 0 and Cycle 1 for studies of star formation. Focusing on nearby star-forming cores where we have the highest spatial resolution, I shall discuss how ALMA will probe the magneto-hydrodynamics of infall/collapse and will constrain the structure of the inner envelope and disk. I shall also discuss important issues (i.e. appropriate dust opacities, etc.) that must be considered in radiative transfer modeling of ALMA observations.

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