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Rollins, RP,Rawlings, JMC,Williams, DA,Redman, MP
2014
October
Monthly Notices Of The Royal Astronomical Society
Champagne flutes and brandy snifters: modelling protostellar outflow-cloud chemical interfaces
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Altmetric: 3WOS: 4 ()
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astrochemistry ISM: jets and outflows ISM: molecules YOUNG STELLAR OBJECTS HCO+ EMISSION CHEMISTRY CIRCUMSTELLAR SPECTROSCOPY ENVELOPES COLLAPSE DATABASE ORIGIN WATER
443
3033
3043
A rich variety of molecular species has now been observed towards hot cores in star-forming regions and in the interstellar medium. An increasing body of evidence from millimetre interferometers suggests that many of these form at the interfaces between protostellar outflows and their natal molecular clouds. However, current models have remained unable to explain the origin of the observational bias towards wide-angled 'brandy snifter' shaped outflows over narrower 'champagne flute' shapes in carbon monoxide imaging. Furthermore, these wide-angled systems exhibit unusually high abundances of the molecular ion HCO+. We present results from a chemodynamic model of such regions where a rich chemistry arises naturally as a result of turbulent mixing between cold, dense molecular gas and the hot, ionized outflow material. The injecta drives a rich and rapid ion-neutral chemistry in qualitative and quantitative agreement with the observations. The observational bias towards wide-angled outflows is explained naturally by the geometry-dependent ion injection rate causing rapid dissociation of CO in the younger systems.
10.1093/mnras/stu1347
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