Hostname: page-component-745bb68f8f-v2bm5 Total loading time: 0 Render date: 2025-02-11T06:05:07.504Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
Rendong Nan
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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