Unified models of molecular emission from Class o 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:	Monthly notices of the Royal Astronomical Society 2013-10, Vol.435 (1), p.289
Hauptverfasser:	Rawlings, J MC, Redman, M P, Carolan, P B
Format:	Artikel
Sprache:	eng
Schlagworte:	Approximation Molecules Star & galaxy formation
Online-Zugang:	Volltext
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