Oleg Y. Gnedin et al. 2005 ApJ 634 344 doi:10.1086/496958
Oleg Y. Gnedin1, Andrew Gould1, Jordi Miralda-Escudé1 and Andrew R. Zentner2
Show affiliationsPrecise proper-motion measurements (σμ ~ 10 μas yr-1) of the recently discovered hypervelocity star (HVS) SDSS J090745.0+024507 would yield significant constraints on the axis ratios and orientation of a triaxial model for the Galactic halo. Triaxiality of dark matter halos is predicted by cold dark matter models of galaxy formation and may be used to probe the nature of dark matter. However, unless the distance to this star is determined to better than 10%, these constraints suffer from one-dimensional degeneracies, which we quantify. We show how proper-motion measurements of several HVSs could simultaneously resolve the distance degeneracies of all such stars and produce a detailed picture of the triaxial halo. Additional HVSs may be found from radial velocity surveys or from parallax/proper-motion data derived from Gaia. High-precision proper-motion measurements of these stars using the Space Interferometry Mission (SIM PlanetQuest) would substantially tighten the constraints they yield on the Galactic potential.
cosmology: theory; dark matter; galaxies: formation; galaxies: halos; Galaxy: halo
Issue 1 (2005 November 20)
Received 2005 June 30, accepted for publication 2005 August 4
Oleg Y. Gnedin et al. 2005 ApJ 634 344
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