4.7 Article

The M31 Velocity Vector. II. Radial Orbit Towards the Milky Way and Implied Local Group Mass

Journal

ASTROPHYSICAL JOURNAL
Volume 753, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/753/1/8

Keywords

galaxies: kinematics and dynamics; Local Group; M31

Funding

  1. National Junior Research Fellowship
  2. Hi Seoul Science Fellowship from Seoul Scholarship Foundation
  3. Basic Science Research Program through the National Research Foundation of Korea
  4. Ministry of Education, Science and Technology [2010-0021558]
  5. KAKENHI [21540247]
  6. W.M. Keck Foundation
  7. Subaru Telescope
  8. National Research Foundation of Korea [2010-0021558] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)
  9. Division Of Astronomical Sciences
  10. Direct For Mathematical & Physical Scien [1009882, 1010039] Funding Source: National Science Foundation
  11. Grants-in-Aid for Scientific Research [21540247] Funding Source: KAKEN

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We determine the velocity vector of M31 with respect to the Milky Way and use this to constrain the mass of the Local Group, based on Hubble Space Telescope proper-motion measurements of three fields presented in Paper I. We construct N-body models for M31 to correct the measurements for the contributions from stellar motions internal to M31. This yields an unbiased estimate for the M31 center-of-mass motion. We also estimate the center-of-mass motion independently, using the kinematics of satellite galaxies of M31 and the Local Group, following previous work but with an expanded satellite sample. All estimates are mutually consistent, and imply a weighted average M31 heliocentric transverse velocity of (nu(W), nu(N)) = (-125.2 +/- 30.8,-73.8 +/- 28.4) kms(-1). We correct for the reflex motion of the Sun using the most recent insights into the solar motion within the Milky Way, which imply a larger azimuthal velocity than previously believed. This implies a radial velocity of M31 with respect to the Milky Way of V-rad,V-M31 = -109.3 +/- 4.4 km s(-1), and a tangential velocity V-tan,V-M31 = 17.0 km s(-1), with 1 sigma confidence region V-tan,V-M31 <= 34.3 km s(-1). Hence, the velocity vector of M31 is statistically consistent with a radial (head-on collision) orbit towards the Milky Way. We revise prior estimates for the Local Group timing mass, including corrections for cosmic bias and scatter, and obtain M-LG M-MW,M-vir+M-M31,M-vir=(4.93 +/- 1.63)x10(12) M-circle dot. Summing known estimates for the individual masses of M31 and the Milky Way obtained from other dynamical methods yields smaller uncertainties. Bayesian combination of the different estimates demonstrates that the timing argument has too much (cosmic) scatter to help much in reducing uncertainties on the Local Group mass, but its inclusion does tend to increase other estimates by similar to 10%. We derive a final estimate for the Local Group mass from literature and new considerations of M-LG = (3.17 +/- 0.57)x10(12) M-circle dot. The velocity and mass results imply at 95% confidence that M33 is bound to M31, consistent with expectation from observed tidal deformations.

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