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Filamentary structure formation in the Interstellar Radiation Field (ISRF)

Published online by Cambridge University Press:  21 March 2013

Jingqi Miao ,
M. Lieu ,
Philip Cox ,
Tim Kinnear  and
Paul Cornwall
Jingqi Miao
Affiliation:
Centre for Astrophysics and Planetary Science (CAPS) University of Kent, CT2 7NH, United Kingdom email: j.miao@kent.ac.uk
M. Lieu
Affiliation:
Centre for Astrophysics and Planetary Science (CAPS) University of Kent, CT2 7NH, United Kingdom email: j.miao@kent.ac.uk
Philip Cox
Affiliation:
Centre for Astrophysics and Planetary Science (CAPS) University of Kent, CT2 7NH, United Kingdom email: j.miao@kent.ac.uk
Tim Kinnear
Affiliation:
Centre for Astrophysics and Planetary Science (CAPS) University of Kent, CT2 7NH, United Kingdom email: j.miao@kent.ac.uk
Paul Cornwall
Affiliation:
Centre for Astrophysics and Planetary Science (CAPS) University of Kent, CT2 7NH, United Kingdom email: j.miao@kent.ac.uk
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Abstract

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A new mechanism is proposed for the formation of filament/core structure by ISRF and clumpy molecular cloud interaction. The derived characterizes of the filament/core network is consistent with that produced by the compressive forcing turbulence model.

Keywords

ISM: clouds — ISM: evolution — ISM: structure
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. 52
Copyright
Copyright © International Astronomical Union 2013

References

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