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20 April 2024
 
  » arxiv » 1602.3180

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Isotropic at the Break? 3D Kinematics of Milky Way Halo Stars in the Foreground of M31
Emily C. Cunningham ; Alis J. Deason ; Puragra Guhathakurta ; Constance M. Rockosi ; Roeland P. van der Marel ; Elisa Toloba ; Karoline M. Gilbert ; Sangmo Tony Sohn ; Claire E. Dorman ;
Date 9 Feb 2016
AbstractWe present the line-of-sight (LOS) velocities for 13 distant main sequence Milky Way halo stars with published proper motions. The proper motions were measured using long baseline (5-7 years) multi-epoch HST/ACS photometry, and the LOS velocities were extracted from deep (5-6 hour integrations) Keck II/DEIMOS spectra. We estimate the parameters of the velocity ellipsoid of the stellar halo using a Markov chain Monte Carlo ensembler sampler method. The velocity second moments in the directions of the Galactic $(l,b,$ LOS) coordinate system are $langle v^2_l angle^{1/2} = 138^{+43}_{-26}$ km/s, $langle v^2_b angle^{1/2} = 88^{+28}_{-17}$ km/s, and $langle v^2_{ m{LOS}} angle^{1/2} = 91^{+27}_{-14}$ km/s. We use these ellipsoid parameters to constrain the velocity anisotropy of the stellar halo. Ours is the first measurement of the anisotropy parameter $eta$ using 3D kinematics outside of the solar neighborhood. We find $eta=-0.3^{+0.4}_{-0.9}$, consistent with isotropy and lower than solar neighborhood $eta$ measurements by 2$sigma$ ($eta_{SN} sim 0.5-0.7$). We identify two stars in our sample that are likely members of the known TriAnd substructure, and excluding these objects from our sample increases our estimate of the anisotropy to $eta=0.1^{+0.4}_{-1.0}$, which is still lower than solar neighborhood measurements by $1sigma$. The potential decrease in $eta$ with Galactocentric radius is inconsistent with theoretical predictions, though consistent with recent observational studies, and may indicate the presence of large, shell-type structure (or structures) at $r sim 25$ kpc. The methods described in this paper will be applied to a much larger sample of stars with 3D kinematics observed through the ongoing HALO7D program.
Source arXiv, 1602.3180
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