Unified Models of Molecular Emission from Class 0 Protostellar Outflow Sources

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 applicabil...

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Veröffentlicht in:	arXiv.org 2013-08
Hauptverfasser:	Rawlings, J M C, Redman, M P, Carolan, P B
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrochemistry Low mass stars Mathematical models Molecular gases Organic chemistry Outflow Parameters Physical properties Physics - Astrophysics of Galaxies Protostars Radiative transfer Star formation Three dimensional models
Online-Zugang:	Volltext
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