首页> 外文期刊>The Astrophysical journal >THE M31 VELOCITY VECTOR. II. RADIAL ORBIT TOWARD THE MILKY WAY AND IMPLIED LOCAL GROUP MASS
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THE M31 VELOCITY VECTOR. II. RADIAL ORBIT TOWARD THE MILKY WAY AND IMPLIED LOCAL GROUP MASS

机译:M31速度矢量。二。径向轨道走向银河系和隐含的局部群质量

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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 (vW , vN ) = (– 125.2 ± 30.8, –73.8 ± 28.4) km s–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, M31 = –109.3 ± 4.4 km s–1, and a tangential velocity of V tan, M31 = 17.0 km s–1, with a 1σ confidence region of V tan, M31 ≤ 34.3 km s–1. Hence, the velocity vector of M31 is statistically consistent with a radial (head-on collision) orbit toward 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, vir + M M31, vir = (4.93 ± 1.63) × 1012 M ☉. 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 ~10%. We derive a final estimate for the Local Group mass from literature and new considerations of M LG = (3.17 ± 0.57) × 1012 M ☉. The velocity and mass results at 95% confidence imply that M33 is bound to M31, consistent with expectation from observed tidal deformations.
机译:我们根据哈勃太空望远镜对论文I中介绍的三个场的固有运动测量,确定相对于银河系的M31速度矢量,并使用它来约束本地群的质量。我们为M31构建N体模型校正测量值以补偿M31内部恒星运动的影响。这样就得出了M31质心运动的无偏估计。我们还根据先前的工作,但使用扩展的卫星样本,使用M31和本地群的卫星星系的运动学独立估计了质心运动。所有估计相互一致,并且意味着加权平均M31日心向横向速度(vW,vN)=(– 125.2±30.8,–73.8±28.4)km s-1。我们使用对银河系中太阳运动的最新见解来校正太阳的反射运动,这暗示着比以前认为的更大的方位角速度。这意味着相对于V rad的银河系,M31的径向速度M31 = –109.3±4.4 km s-1,而V tan的切线速度M31 = 17.0 km s-1,其1σ置信区间为V tan,M31≤34.3 km s–1。因此,M31的速度矢量在统计上与朝向银河系的径向(正面碰撞)轨道一致。我们修改了对本地组定时质量的先前估计,包括对宇宙偏差和散射的校正,并获得M LG≡M MW,vir + M M31,vir =(4.93±1.63)×1012 M☉。对其他动力学方法获得的M31和银河系单个质量的已知估计值进行汇总得出的不确定性较小。不同估计值的贝叶斯组合表明,时间论点具有太多(宇宙)分散性,无法帮助减少本地组质量的不确定性,但是将其包含进来确实会使其他估计值增加约10%。我们从文献和M LG =(3.17±0.57)×1012 M new的新考虑中得出对本地群质量的最终估计。 95%置信度下的速度和质量结果表明M33与M31绑定,这与观察到的潮汐变形一致。

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