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Phil Marshall

Broken Degeneracies: The Rotation Curve and Velocity Anisotropy of the Milky Way Halo - 0 views

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    Deason et al have an improved measurement of density and velocities of blue horizontal branch stars in the MW halo: here they fit dynamical models an infer a halo of about 1e12 Msun (as before) and quite a high concentration (cvir~20). Since concentration reflects age, this is consistent with the picture in which the MW has been undisturbed for a long time.
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