Fading Features Found in the Kinematics of the Far-Reaching Milky Way Stellar Halo
arXiv:1507.00351 · doi:10.1093/mnras/stv1448
Abstract
We test the long-term kinematical stability of a Galactic stellar halo model, due to Kafle, et al. (2012), who study the kinematics of approximately 5000 blue horizontal branch (BHB) stars in the Sloan Digital Sky Survey (SDSS). The velocity dispersion and anisotropy parameter of the stars have been determined as functions of Galactocentric radius, over the range kpc, and show a strong dip in the anisotropy profile at kpc. By directly integrating orbits of particles in a 3-D model of the Galactic potential with these characteristics, we show that the and profiles quickly evolve on a time scale of a Myr whereas the density profile remains largely unaffected. We suggest that the feature is therefore transient. The origin of such features in the Galactic halo remains unclear.
Accepted for publication in MNRAS, 5 pages, 4 figures, 1 table
References in corpus (5)
Cited by in corpus (5)
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- Galactic googly: the rotation-metallicity bias in the inner stellar halo of the Milky Way
- The Milky Way Revealed by Variable Stars I: Sample Selection of RR Lyrae stars, and Evidence for the Merger History
- Probing the Galactic halo with RR Lyrae stars -- IV. On the Oosterhoff dichotomy of RR Lyrae stars