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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(437), p. 415-423, 2013

DOI: 10.1093/mnras/stt1891

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The dependence of dark matter profiles on the stellar-to-halo mass ratio: a prediction for cusps versus cores

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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