The ISM in spiral galaxies: can cooling in spiral shocks produce molecular clouds?
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/389/3/1097/3321311/mnras0389-1097.pdf
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1. Large-scale dissociation of molecular gas in galaxies by newly formed stars
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4. Turbulent Flow–driven Molecular Cloud Formation: A Solution to the Post–T Tauri Problem?
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