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Spectroscopic signatures of infall in young protostellar systems
The Astrophysical Journal1994Vol. 431, pp. 767–767
Citations Over TimeTop 10% of 1994 papers
Abstract
We present the first radiative transfer calculations of millimeter and submillimeter molecular line emission from 'self-consistent' models of nonspherical, collapsing, rotating protostellar systems. We find that: (1) the morphology of the gas and dust emission is a strong function of collapse time and angular resolution, (2) centroid velocity maps can provide a distinct infall signature, and (3) the unambiguous detection of infall toward binary systems becomes more difficult with increasing binary separation.
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