论文标题
长期彗星运动的恒星珀尔特(Stellar Perturber)列表中的更新清单中的一个惊喜
A surprise in the updated list of stellar perturbers of long period comets motion
论文作者
论文摘要
第二个GAIA数据发布(GAIA DR2)为我们提供了13亿个来源的精确的五参数天文学。由于恒星通过太阳系接近太阳系被认为是影响长期彗星的动态历史的原因,我们更新并扩展了可能会扰乱这些彗星运动的恒星列表。我们的目标是宣布一个公开可用的数据库,其中包含可能会扰乱长期彗星运动的恒星和恒星系统的最新列表。我们添加了新对象并修订了先前发布的列表。特别重点是恒星系统。包括有关群众估计的讨论。最好使用来自Gaia DR2的天文标准,并增强了来自其他来源的数据,我们计算每个恒星的空间位置和速度。为了根据其最小的中心距离进行过滤研究的对象,我们在银河电位及其相互作用下数值整合了恒星的运动。我们宣布了彗星运动的恒星珀特伯的更新列表,包括Persturbers的群众以及公开可用的数据库接口。这些数据已准备好与观察到的长期彗星轨道一起使用,以研究整个Perturbers或特定恒星对特定彗星的动态过去或未来的个人影响。与先前发表的资料相比,添加了147个新的Perturbers。我们证明,一组新的潜在遗物构成了研究彗星动力学研究的重要工具。数据的使用显着改变了过去和将来的彗星运动分析的结果。我们指出了我们列表中的一个令人困惑的物体ALS9243。GaiaDR2天文统计表明,这颗星星与太阳的恒星非常紧密地相遇,但其天体物理参数导致ALS 9243的当前距离完全不同。
The second Gaia data release (Gaia DR2) provided us with the precise five-parameter astrometry for 1.3 billion of sources. As stars passing close to the Solar System are thought to be responsible for influencing the dynamical history of long period comets, we update and extend the list of stars that could potentially perturb motion of these comets. We aim to announce a publicly available database containing an up to date list of stars and stellar systems potentially perturbing long period comets motion. We add new objects and revise previously published lists. Special emphasis was placed on stellar systems. Discussion on masses estimation is included. Using the astrometry, preferably from Gaia DR2, augmented with data from other sources, we calculate spatial positions and velocities for each star. To filter studied objects on the basis of their minimal heliocentric distances we numerically integrate motion of stars under the Galactic potential and their mutual interactions. We announce the updated list of stellar perturbers of cometary motion, including masses of perturbers along with the publicly available database interface. These data are ready to be used with the observed long period comets orbits to study an individual influence of a whole sample of perturbers, or specific stars, on a dynamical past or future of a specific comet. 147 new perturbers were added in comparison to the previously published sources. We demonstrate that a new set of potential perturbers constitute an important tool in studies of cometary dynamics. The usage of our data significantly changes results of the past and future comet motion analysis. We point out a puzzling object in our list, star ALS 9243. The Gaia DR2 astrometry suggests a very close encounter of this star with the Sun however, its astrophysical parameters result in a completely different current distance of ALS 9243 and its large mass.