Chemical evolution of galaxies with radiation-driven dust wind
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/444/4/3879/6362600/stu1731.pdf
Reference73 articles.
1. Enrichment of the Intergalactic Medium by Radiation Pressure–driven Dust Efflux
2. Coevolution of dust, gas and stars in galaxies – I. Spatial distributions and scaling-relations of dust and molecular hydrogen
3. CHEMICAL EVOLUTION OF THE LARGE MAGELLANIC CLOUD
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4. The formation of S0 galaxies with counter-rotating neutral and molecular hydrogen;Monthly Notices of the Royal Astronomical Society;2017-05-03
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