太阳附近盘状恒星的运动学

A. Gómez, S. Grenier, S. Udry, M. Haywood, V. Sabas, L. Meillon, F. Royer, Y. Lebreton
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引用次数: 7

摘要

利用数千颗B-F型恒星的希巴谷视差和固有运动以及径向速度补充数据(Coravel用于晚期恒星,新的地面数据用于早期恒星),确定了速度椭球作为年龄的函数。估计了速度色散比、顶点偏差和年龄-速度色散关系(AVR)随年龄的变化。我们的结果证实,混合在约0:8时并不完全。1 Gyr。速度椭球的形状随时间变化,从最大值开始逐渐变圆,此后基本保持不变;在大约4 ?之后,磁盘没有动态的显著演化。5 Gyr。垂直于银道平面方向上的速度色散在15?薄盘星的直径为17公里。顶点偏差随着年龄的增长而下降,在5gyr后保持在零附近。
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Kinematics of Disk Stars in the Solar Neighbourhood
Using Hipparcos parallaxes and proper motions together with radial velocity complementary data (Coravel for late type stars and new ground-based data for early type stars) for several thousand B-F type stars, the velocity ellipsoid has been determined as a function of age. The variations with age of the ratio of the velocity dispersions, of the vertex deviation and the age-velocity dispersion relation (AVR) have been estimated. Our results connrm that mixing is not complete at about 0:8 ? 1 Gyr. The shape of the velocity ellipsoid changes with time, getting rounder from a maximum, thereafter remaining roughly constant; there is no dynamically signiicant evolution of the disk after about 4 ? 5 Gyr. The velocity dispersion in the direction perpendicular to the galactic plane saturates at about 15?17 km s ?1 for thin disk stars. The vertex deviation declines with age and remains near zero after 5 Gyr.
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