Modeling Line Profiles of Protostellar Collapse with Rotation

Details Modeling Line Profiles of Protostellar Collapse with Rotation Modeling Line Profiles of Protostellar Collapse with Rotation

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...185.8418c&link_type=abstract

American Astronomical Society, 185th AAS Meeting, #84.18; Bulletin of the American Astronomical Society, Vol. 26, p.1459

Astronomy and Astrophysics

Astronomy

Scientific paper

We developed a two-dimensional radiative transfer code using the Monte
Carlo method. This code assumes the cloud has an azimuthal symmetry.
With this code, we generated several molecular line profiles from
protostellar collapse models including rotation, and compared the result
with observations.

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