Formation of a counter-rotating stellar population in the Large Magellanic Cloud: a Magellanic triplet system?
Author:
Affiliation:
1. International Centre for Radio Astronomy Research/The University of Western Australia, M468, 35 Stirling Hwy, Crawley WA 6009, Australia
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/480/1/L141/25644728/sly143.pdf
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1. Simulating galaxy evolution with a non-universal stellar initial mass function
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4. Dynamical Influences of the Last Magellanic Interaction on the Magellanic Clouds
5. The total mass and dark halo properties of the Small Magellanic Cloud
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