Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 4(380), p. 1669-1677, 2007
DOI: 10.1111/j.1365-2966.2007.12219.x
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On the origin of the kinematical differences between the stellar halo and the old globular cluster system in the Large Magellanic Cloud
Journal article published in 2007 by
Kenji Bekki 
This paper was not found in any repository, but could be made available legally by the author.
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