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Rawlings, JMC,Redman, MP,Carolan, PB
2013
October
Monthly Notices Of The Royal Astronomical Society
Unified models of molecular emission from Class 0 protostellar outflow sources
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line: profiles radiative transfer stars: formation stars: protostars stars: winds, outflows ISM: molecules YOUNG STELLAR OBJECTS SMALL-SCALE STRUCTURE LOW-MASS PROTOSTARS SUBMILLIMETER CONTINUUM OBSERVATIONS STAR-FORMATION RADIATIVE-TRANSFER DARK CLOUD BIPOLAR OUTFLOW LINE-PROFILES DENSE CORES
435
289
302
Low-mass star-forming regions are more complex than the simple spherically symmetric approximation that is often assumed. We apply a more realistic infall/outflow physical model to molecular/continuum observations of three late Class 0 protostellar sources with the aims of (a) proving the applicability of a single physical model for all three sources and (b) deriving physical parameters for the molecular gas component in each of the sources. We have observed several molecular species in multiple rotational transitions. The observed line profiles were modelled in the context of a dynamical model which incorporates infall and bipolar outflows, using a three-dimensional radiative transfer code. This results in constraints on the physical parameters and chemical abundances in each source. Self-consistent fits to each source are obtained. We constrain the characteristics of the molecular gas in the envelopes as well as in the molecular outflows. We find that the molecular gas abundances in the infalling envelope are reduced, presumably due to freeze-out, whilst the abundances in the molecular outflows are enhanced, presumably due to dynamical activity. Despite the fact that the line profiles show significant source-to-source variation, which primarily derives from variations in the outflow viewing angle, the physical parameters of the gas are found to be similar in each core.
DOI 10.1093/mnras/stt1295
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