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Feedback of outflows in the Taurus Molecular Cloud

Published online by Cambridge University Press:  21 March 2013

Huixian Li ,
Di Li  and
Rendong Nan
Huixian Li
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Di Li
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China Space Science Institute, Boulder, CO email: lhx@nao.cas.cn
Rendong Nan
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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Abstract

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We collected 27 outflows from the literature and found 8 new ones in the FCRAO CO maps of the Taurus molecular cloud. The total kinetic energy of the 35 outflows is found to be about 3% of the gravitational potential energy from the whole cloud. The feedback effect due to the outflows is minor in Taurus.

Keywords

ISM: clouds — ISM: jets and outflows — ISM: individual (Taurus)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 47
Copyright
Copyright © International Astronomical Union 2013

References

Goldsmith, P. F., Heyer, M., Narayanan, G., Snell, R., Li, D., & Brunt, C. 2008, ApJ, 680, 428Google Scholar