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Q56907286-9C3C776D-11B8-464D-9EE1-1C7C06A6ADE8
Q56907286-9C3C776D-11B8-464D-9EE1-1C7C06A6ADE8
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http://www.wikidata.org/entity/statement/Q56907286-9C3C776D-11B8-464D-9EE1-1C7C06A6ADE8
What to expect from dynamical modelling of galactic haloes
P2860
Q56907286-9C3C776D-11B8-464D-9EE1-1C7C06A6ADE8
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http://www.wikidata.org/entity/statement/Q56907286-9C3C776D-11B8-464D-9EE1-1C7C06A6ADE8
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eb050230e29e31a61a3210f0019857d7cb4ca01b
P2860
Filamentary accretion cannot explain the orbital poles of the Milky Way satellites