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- W4299703065 abstract "The origin of high velocity stars observed in the halo of our Galaxy is still unclear. In this work we test the hypothesis, raised by results of recent high precision $N$-body simulations, of strong acceleration of stars belonging to a massive globular cluster orbitally decayed in the central region of the host galaxy where it suffers of a close interaction with a super massive black hole, which, for these test cases, we assumed $10^8$ M$_odot$ in mass." @default.
- W4299703065 created "2022-10-02" @default.
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- W4299703065 date "2015-07-02" @default.
- W4299703065 modified "2023-09-30" @default.
- W4299703065 title "Super Massive Black Holes and the Origin of High-Velocity Stars" @default.
- W4299703065 doi "https://doi.org/10.48550/arxiv.1507.00520" @default.
- W4299703065 hasPublicationYear "2015" @default.
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