Sheets, filaments, and clumps – high-resolution simulations of how the thermal instability can form molecular clouds
Author:
Affiliation:
1. School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK
2. School of Mathematics, University of Leeds, Leeds LS2 9JT, UK
Funder
Science and Technology Facilities Council
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/485/4/4686/28227960/stz768.pdf
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1. Characterizing the properties of nearby molecular filaments observed with Herschel
2. THE THERMALLY UNSTABLE WARM NEUTRAL MEDIUM: KEY FOR MODELING THE INTERSTELLAR MEDIUM
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