Abstract
BHR 71 is a well isolated Bok globule located at ~200 pc, which harbours a highly collimated bipolar outflow. The outflow is driven by a very young Class 0 protostar with a luminosity of ~9 L_sun. It is one of a very small number that show enhanced abundances of a number of molecular species, notably SiO and CH3OH, due to shock processing of the ambient medium. In this paper the properties of the globule and outflow are discussed.
Cite
CITATION STYLE
APA
Bourke, T. L. (2006). The Spectacular BHR 71 Outflow. In The Origin of Stars and Planets: The VLT View (pp. 247–252). Springer-Verlag. https://doi.org/10.1007/10856518_31
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