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High velocity stars are stars moving at velocities so high to require an acceleration mechanism involving binary systems or the presence of a massive central black hole. In the frame of a galaxy hosting a supermassive black hole binary (of…

星系天体物理 · 物理学 2016-03-23 Giacomo Fragione , Roberto Capuzzo-Dolcetta

One possible origin of high velocity stars in the Galaxy is that they are the product of the interaction of binary systems and supermassive black holes. We investigate a new production channel of high velocity stars as due to the close…

星系天体物理 · 物理学 2016-06-14 Giacomo Fragione , Roberto Capuzzo-Dolcetta

Observations show the presence, in the halo of our Galaxy, of stars moving at velocities so high to require an acceleration mechanism involving the presence of a massive central black hole. Thus, in the frame of a galaxy hosting a…

星系天体物理 · 物理学 2015-10-21 R. Capuzzo-Dolcetta , G. Fragione

In recent years surveys have identified several dozen B stars in the Milky Way halo moving faster than the local escape speed. The origin of most of these hypervelocity stars (HVSs) is still poorly constrained. Here we show that the…

星系天体物理 · 物理学 2023-01-02 Aleksey Generozov , Hagai B. Perets

Hypervelocity stars (HVSs) are stars ejected completely out of the Milky Way by three-body interactions with the massive black hole in the Galactic center. We describe 643 new spectroscopic observations from our targeted survey for HVSs. We…

Hypervelocity stars (HVSs) represent a unique population of stars in the Galaxy reflecting properties of the whole Galactic potential. Determining their origin is of fundamental importance to constrain the shape and mass of the dark halo.…

星系天体物理 · 物理学 2019-09-25 Giacomo Fragione , Alessia Gualandris

Hypervelocity stars (HVSs) that are observed in the Galactic halo, are believed to be accelerated to large velocities by a process of tidal disruption of binary stars passing close to a supermassive black hole (SMBH) which resides in the…

星系天体物理 · 物理学 2016-09-28 Ladislav Subr , Jaroslav Haas

The hypervelocity stars recently found in the Galactic halo are expelled from the Galactic center through interactions between binary stars and the central massive black hole or between single stars and a hypothetical massive binary black…

天体物理学 · 物理学 2011-05-19 Youjun Lu , Qingjuan Yu , D. N. C. Lin

Stars within 0.1 pc of the supermassive black hole Sgr A* at the Galactic centre are expected to encounter a cluster of stellar-mass black holes (BHs) that have segregated to that region. Some of these stars will scatter off an orbiting BH…

天体物理学 · 物理学 2008-07-15 Ryan M. O'Leary , Abraham Loeb

The discovery of hypervelocity stars (HVS) leaving our galaxy with speeds of nearly $10^{3}$ km s$^{-1}$ has provided strong evidence towards the existence of a massive compact object at the galaxy's center. HVS ejected via the disruption…

星系天体物理 · 物理学 2015-06-18 James Guillochon , Abraham Loeb

Halo stars with unusually high radial velocity ("hypervelocity" stars, or HVS) are thought to be stars unbound to the Milky Way that originate from the gravitational interaction of stellar systems with the supermassive black hole at the…

天体物理学 · 物理学 2009-11-13 Mario G. Abadi , Julio F. Navarro , Matthias Steinmetz

Recent surveys have identified seven hypervelocity stars (HVSs) in the halo of the Milky Way. Most of these stars may have originated from the breakup of binary star systems by the nuclear black hole SgrA*. In some instances, the breakup of…

天体物理学 · 物理学 2008-11-26 Idan Ginsburg , Abraham Loeb

The most commonly accepted explanation for the origin of hypervelocity stars in the halo of the Milky Way is that they are the result of tidal disruption of binaries by the massive black hole at the center of the Galaxy. We show that, if…

天体物理学 · 物理学 2009-11-13 Brad Hansen

We consider the process of stellar binaries tidally disrupted by a supermassive black hole. For highly eccentric orbits, as one star is ejected from the three-body system, the companion remains bound to the black hole. Hypervelocity stars…

星系天体物理 · 物理学 2015-06-16 Elena M. Rossi , Shiho Kobayashi , Re'em Sari

We performed numerical simulations of dynamical encounters between hard massive binaries and a very massive star (VMS; formed through runaway mergers of ordinary stars in the dense core of a young massive star cluster), in order to explore…

太阳与恒星天体物理 · 物理学 2015-05-14 V. V. Gvaramadze , A. Gualandris , S. Portegies Zwart

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…

星系天体物理 · 物理学 2015-07-03 Roberto Capuzzo-Dolcetta , Giacomo Fragione

Young massive stars in the halo are assumed to be runaway stars from the Galactic disk. Possible ejection scenarios are binary supernova ejections (BSE) or dynamical ejections from star clusters (DE). Hypervelocity stars (HVSs) are extreme…

太阳与恒星天体物理 · 物理学 2018-12-05 Andreas Irrgang , Simon Kreuzer , Ulrich Heber

Hypervelocity stars (HVSs) are a natural consequence of the presence of a massive nuclear black hole (Sgr A*) in the Galactic Center. Here we use the Brown et al. sample of unbound and bound HVSs together with numerical simulations of the…

天体物理学 · 物理学 2009-06-23 A. Sesana , F. Haardt , P. Madau

About 20% of all massive stars in the Milky Way have unusually high velocities, the origin of which has puzzled astronomers for half a century. We argue that these velocities originate from strong gravitational interactions between single…

星系天体物理 · 物理学 2015-06-03 Michiko Fujii , Simon Portegies Zwart

Several tens of hyper-velocity stars (HVSs) have been discovered escaping our Galaxy. These stars share a common origin in the Galactic centre and are distributed anisotropically in Galactic longitude and latitude. We examine the…

星系天体物理 · 物理学 2015-06-16 Kastytis Zubovas , Graham A. Wynn , Alessia Gualandris
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