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Velocity Distributions of Runaway Stars Produced by Supernovae in the Galaxy

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Abstract

Using a method of population synthesis, we investigate the runaway stars produced by disrupted binaries via asymmetric core collapse supernova explosions (CC-RASs) and thermonuclear supernova explosions (TN-RASs). We find the velocities of CC-RASs in the range of about 30–100 km s −1. The runaway stars observed in the galaxy are possibly CC-RASs. Due to differences in stellar chemical components and structures, TN-RASs are divided into hydrogen-rich TN-RASs and helium-rich TN-RASs. The velocities of the former are about 100–500 km s −1, while the velocities of the latter are mainly between 600 and 1100 km s −1. The hypervelocity stars observed in the galaxy may originate from thermonuclear supernova explosions. Our results possibly cover the US 708 which is a compact helium star and travels with a velocity of 1157 ±53 km s−1 in our galaxy.

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Acknowledgements

This work was supported by XinJiang Science Fund for Distinguished Young Scholars under Nos 2014721015 and 2013721014, the National Natural Science Foundation of China under Nos 11473024, 11363005 and 11163005.

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Correspondence to Abudusaimaitijiang Yisikandeer.

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Yisikandeer, A., Zhu, C., Wang, Z. et al. Velocity Distributions of Runaway Stars Produced by Supernovae in the Galaxy. J Astrophys Astron 37, 22 (2016). https://doi.org/10.1007/s12036-016-9400-2

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  • DOI: https://doi.org/10.1007/s12036-016-9400-2

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