论文标题
盖亚(Gaia)的当地群体质量
The Local Group Mass in the light of Gaia
论文作者
论文摘要
现在已经由{\ it Gaia}卫星提供了高精度的M31和其他本地组卫星的适当动作(PMS)。我们重新审视定时论点,以从银河系和M31的轨道计算本地群体的总质量$ m $,从而允许宇宙常数。我们纠正了由大麦芽云(LMC)的存在引起的系统效应。 LMC与银河系的相互作用引起了向LMC的运动。必须删除对银河系和M31进近速度的这种贡献。我们通过提取针对本地群体积聚史的校正因子提取校正因子而允许宇宙偏见和散射。校正因子的分布以$ 0.63 $为中心,散布$ \ pm 0.2 $,这表明计时论点显着高估了真正的质量。调整所有这些效果,本地组的估计质量为$ m = 3.4^{+1.4} _ { - 1.1} \ times 10^{12} M _ {\ odot} $(68%Cl)使用M31切向速度$ 82^{+38} {+38} _ {+38} _ { - 35} $ s时。 $ 59^{+42} _ { - 38} $ km/s(从相同的PM数据衍生而上的与切向速度平坦的同一PM数据衍生导致估计的质量为$ M = 3.1^{+1.3} _ { - 1.0} { - 1.0} \ times 10^{12} m _ _} $ ODOT。通过库存与4个最重要的LG成员(银河系,M31,M33和LMC)相关的总质量,我们估计已知的质量在$ 3.7^{+0.5} _ { - 0.5} _ { - 0.5} \ times 10^{12} {12}} \,m _ {\ odot} $。
High accuracy proper motions (PMs) of M31 and other Local Group satellites have now been provided by the {\it Gaia} satellite. We revisit the Timing Argument to compute the total mass $M$ of the Local Group from the orbit of the Milky Way and M31, allowing for the Cosmological Constant. We rectify for a systematic effect caused by the presence of the Large Magellanic Cloud (LMC). The interaction of the LMC with the Milky Way induces a motion towards the LMC. This contribution to the measured velocity of approach of the Milky Way and M31 must be removed. We allow for cosmic bias and scatter by extracting correction factors tailored to the accretion history of the Local Group. The distribution of correction factors is centered around $0.63$ with a scatter $\pm 0.2$, indicating that the Timing Argument significantly overestimates the true mass. Adjusting for all these effects, the estimated mass of the Local Group is $ M = 3.4^{+1.4}_{-1.1} \times 10^{12} M_{\odot}$ (68 % CL) when using the M31 tangential velocity $ 82^{+38}_{-35}$ km/s. Lower tangential velocity models with $59^{+42}_{-38}$ km/s (derived from the same PM data with a flat prior on the tangential velocity) lead to an estimated mass of $ M = 3.1^{+1.3}_{-1.0} \times 10^{12} M_{\odot}$ (68 % CL). By making an inventory of the total mass associated with the 4 most substantial LG members (the Milky Way, M31, M33 and the LMC), we estimate the known mass is in the range $3.7^{+0.5}_{-0.5} \times 10^{12} \, M_{\odot}$.