The spectacular BHR 71 outflow

被引：1
作者：
Bourke, TL [1 ]
机构：
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
来源：
ORIGINS OF STARS AND PLANETS: THE VLT VIEW | 2002年
关键词：
D O I：
10.1007/10856518_31
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
BHR 71 is a well isolated Bok globule located at similar to200 pc, which harbours a highly collimated bipolar outflow. The outflow is driven by a very young Class 0 protostar with a luminosity of similar to9 L-circle dot. 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.
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页码：247 / 252
页数：6
相关论文
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