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Hypervelocity stars: theory and observations

  a,   b, §  b
a Institute of Astronomy, Russian Academy of Sciences, ul. Pyatnitskaya 48, Moscow, 119017, Russian Federation
b Russian Federal Nuclear Center E.N.Zababakhin All-Russia Scientific Research Institute ofTechnical Physics, PO Box 245, Snezhinsk, Chelyabinsk Region, Russian Federation

Relativistic velocity is a kinematic feature of micro-objects (elementary particles). Their application to macro objects (stars, planets, asteroids, neutron stars, and stellar-mass black holes) is currently under scientific discussion. This potential was recognized after Warren Brown discovered hypervelocity stars (HVSs) at the beginning of the 21st century. Jack Hills predicted these stars in 1988 due to the dynamical capture of a binary star by the central supermassive black hole (SMBH). The acceleration mechanism due to momentum exchange in the classical three-body problem provides the kinetic resource for HVS formation by the gravitational capture of the remaining component. The present threshold of the anomalous stellar kinematics exceeds ~1700 km s−1 and can be reproduced by some mechanisms as alternatives to Hills's scenario. HVSs can arise due to the collisional evolution of stellar clusters, supernova explosions in close binary stars, the orbital instability of triple stars, stellar captures from other galaxies, etc. Scenarios with the participation of black holes with masses ranging from stellar values to several billion solar masses are the most promising for the generation of anomalously high stellar velocities. Hills's scenario has a special place in HVS studies, because, being based on the accidental capture of a binary star by the SMBH, it does not relate to the problem of the galactic center population. This scenario predicts self-consistent statistics of HVSs and captured stars which may be identified with S-stars. The discovery of S-stars played an essential role in studies of the galactic center; their dynamics have independently provided incontestable proof of the SMBH's existence. This review briefly discusses the history of the discovery and investigation of HVSs and S-stars, provides an account of their observational statistics, and describes their modeling methods in the classical three-body and N body problems. We study the limits of the effective acceleration of stars in the classical Hills scenario and the modified mechanism that allows a change of one of the binary components to another SMBH. The acceleration acquired by the star in a mutual field of two SMBHs can produce stars with relativistic velocitie (1/2c—2/3c). Using a self-consistent probabilistic model combining the classical and modified Hills scenarios, we predict the formation probability of HVSs in the Galaxy and of extragalactic stars with relativistic velocities. We discuss the prospects of searches for stars and asteroids with relativistic velocities by future space missions and using new knowledge about the Universe.

Typically, an English fulltext is available in about 3 months from the date of publication of the original article.

Keywords: kinematic anomaly, dynamical capture, Hills's scenario, S-stars, hypervelocity stars, stars with relativistic velocities, supermassive black hole, galaxies
PACS: 95.10.−a, 97.10.Wn, 98.62.Js (all)
DOI: 10.3367/UFNe.2020.11.038892
URL: https://ufn.ru/en/articles/2021/10/a/
Citation: Tutukov A V, Dryomova G N, Dremov V V "Hypervelocity stars: theory and observations" Phys. Usp. 64 967–989 (2021)
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Received: 28th, July 2020, revised: 19th, November 2020, 30th, November 2020

:   ,   ,    « : » 191 1017–1043 (2021); DOI: 10.3367/UFNr.2020.11.038892

References (142) Similar articles (17) ↓

  1. A.V. Tutukov, A.M. Cherepashchuk “Evolution of close binary stars: theory and observations63 209–244 (2020)
  2. P.B. Ivanov, E.V. Mikheeva et alInterferometric observations of supermassive black holes in the millimeter wave band62 423–449 (2019)
  3. V.V. Zhuravlev “Analytical models of relativistic accretion disks58 527–555 (2015)
  4. V.I. Dokuchaev “Birth and life of massive black holes34 (6) 447–470 (1991)
  5. A.G. Doroshkevich, V.N. Lukash, E.V. Mikheeva “A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model55 3–17 (2012)
  6. A.B. Aleksandrov, A.B. Dashkina et alSearch for weakly interacting massive dark matter particles: state of the art and prospects64 861–889 (2021)
  7. V.S. Beskin “Magnetohydrodynamic models of astrophysical jets53 1199–1233 (2010)
  8. I.G. Dymnikova “Motion of particles and photons in the gravitational field of a rotating body (In memory of Vladimir Afanas’evich Ruban)29 215–237 (1986)
  9. A.Y. Potekhin “Atmospheres and radiating surfaces of neutron stars57 735–770 (2014)
  10. Yu.N. Efremov, A.D. Chernin “Large-scale star formation in galaxies46 1–20 (2003)
  11. A.M. Cherepashchuk “Masses of black holes in binary stellar systems39 759–780 (1996)
  12. V.N. Rudenko “Relativistic experiments in gravitational fields21 893–917 (1978)
  13. D.Ya. Martynov “Close binary stars and their significance for the theory of stellar evolution15 786–803 (1973)
  14. A.E. Dubinov, I.Yu. Kornilova, V.D. Selemir “Collective ion acceleration in systems with a virtual cathode45 1109–1129 (2002)
  15. T.I. Belova, A.E. Kudryavtsev “Solitons and their interactions in classical field theory40 359–386 (1997)
  16. M.A. Liberman, B. Johansson “Properties of matter in ultrahigh magnetic fields and the structure of the surface of neutron stars38 117–136 (1995)
  17. V.P. Chechev, Ya.M. Kramarovskii “The theory of nucleosynthesis in stars: the slow neutron capture process24 566–584 (1981)

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