Stellar comet spear

IF 0.4 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Contributions of the Astronomical Observatory Skalnate Pleso Pub Date : 2021-12-01 DOI:10.31577/caosp.2021.51.3.270
M. Sizova, A. Tutukov, S. Vereshchagin
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Abstract

One of the consequences of the evolutionary process of the planetary system is the appearance of comets, asteroids, and even planets (ACP) unbound to their parent star. These small bodies are scattered into interstellar space, orbit the Galactic Center and expand along the star orbit with time. The formed structure resembles a spear in its shape. Similar ACP spears have all stars with planetary systems in the Galaxy. Since such stars are part of the open clusters population, they scatter and form the ACPS spears. In this paper, we performed numerical modeling of the ACP and ASPC spears and estimated their parameters, such as length, width, and time of formation.
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恒星彗星矛
行星系统演化过程的结果之一是彗星、小行星甚至行星(ACP)的出现,这些行星与它们的母恒星脱离了联系。这些小天体分散在星际空间中,围绕银河系中心运行,并随着时间的推移沿着恒星轨道膨胀。形成的结构在形状上类似于矛。类似的ACP矛有银河系中所有具有行星系统的恒星。由于这些恒星是疏散星团的一部分,它们分散形成ACPS矛。在本文中,我们对ACP和ASPC矛进行了数值模拟,并估计了它们的长度、宽度和形成时间等参数。
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来源期刊
CiteScore
1.10
自引率
20.00%
发文量
4
审稿时长
>12 weeks
期刊介绍: Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.
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