The Magellanic squall: gas replenishment from the Small to the Large Magellanic Cloud
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/381/1/L16/3683131/381-1-L16.pdf
Reference20 articles.
1. Formation and evolution of the Magellanic Clouds - I. Origin of structural, kinematic and chemical properties of the Large Magellanic Cloud
2. Dynamical Influences of the Last Magellanic Interaction on the Magellanic Clouds
3. Formation of Star Clusters in the Large Magellanic Cloud and Small Magellanic Cloud. I. Preliminary Results on Cluster Formation from Colliding Gas Clouds
4. Explaining the Mysterious Age Gap of Globular Clusters in the Large Magellanic Cloud
5. Spectroscopy of Red Giants in the Large Magellanic Cloud Bar: Abundances, Kinematics, and the Age-Metallicity Relation
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