识别高速恒星的诞生地:CepOB2 协会

S. Ghazaryan, L. Hambardzumyan, A. Grigoryan, K. Gigoyan, K.-U. Michel, V. Hambaryan, R. Neuhaeuser
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引用次数: 0

摘要

我们搜索了高速恒星(失控恒星、走行恒星、脉冲星、HMXBs 和 LMXBs),它们很可能起源于复杂的 CepOB2 联合体,即其核心(小星团或多个恒星系统)。通过对它们的回溯运动研究,我们发现至少有两对由失控恒星和脉冲星组成的脉冲星,它们出现在 1.5-5.5 Myr 前的 Cep OB2 联合体恒星群中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Identification of birth places of high-velocity stars: CepOB2 association
We have searched high-velocity stars (runaway, walk-away, pulsars, HMXBs and LMXBs), which could have, most probably, originated in the complex CepOB2 association, i.e. in the cores (small clusters or multiple stellar systems) of it. With the trace-back motion study of them we found at least two pairs consisting of a runaway star and pulsar, which were within stellar groups in the Cep OB2 association ∼ 1.5-5.5 Myr ago.
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