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Hypervelocity stars (HVSs) found in the Galactic halo are probably the dynamical products of interactions between (binary) stars and the massive black hole(s) (MBH) in the Galactic center (GC). It has been shown that the detected HVSs are…

星系天体物理 · 物理学 2015-05-28 Fupeng Zhang , Youjun Lu , Qingjuan Yu

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) 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 (HVS) traverse the Galaxy from the central black hole to the outer halo. We show that the Galactic potential within 200 pc acts as a high pass filter preventing low velocity HVS from reaching the halo. To trace the…

天体物理学 · 物理学 2009-11-13 S. J. Kenyon , B. C. Bromley , M. J. Geller , W. R. Brown

Hypervelocity stars (HVSs) are produced by the Hills mechanism when a stellar binary is disrupted by a supermassive black hole (SMBH). The HVS Survey detected 21 unbound B-type main-sequence stars in the Milky Way's outer halo that are…

We have performed N-body simulations of the formation of hyper-velocity stars (HVS) in the centre of the Milky Way due to inspiralling intermediate-mass black holes (IMBHs). We considered IMBHs of different masses, all starting from…

天体物理学 · 物理学 2009-11-11 Holger Baumgardt , Alessia Gualandris , Simon Portegies Zwart

In recent years several hypervelocity stars (HVSs) have been observed in the halo of our Galaxy. Such stars are thought to be ejected through dynamical interactions near the massive black hole (MBH) in the Galactic center. Three scenarios…

天体物理学 · 物理学 2008-12-18 Hagai B. Perets

Hypervelocity stars (HVSs) are stars ejected from the Galactic Centre (GC) through tidal interactions with the central supermassive black hole. Formed in the immediate vicinity of Sgr~A$^\ast$, these stars are accelerated to velocities high…

星系天体物理 · 物理学 2026-05-13 Manuel Cavieres , Sergey E. Koposov , Elena Maria Rossi , Zephyr Penoyre , Sill Verberne

The enormous velocities of the so called hypervelocity stars (HVSs) derive, likely, from close interactions with massive black holes, binary stars encounters or supernova explosions. In this paper, we investigate the origin of hypervelocity…

星系天体物理 · 物理学 2017-01-25 Giacomo Fragione , Roberto Capuzzo-Dolcetta , Pavel Kroupa

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

In this paper, we investigate the link between the hypervelocity stars (HVSs) discovered in the Galactic halo and the S-stars moving in the Galactic center (GC), under the hypothesis that they are both the products of the tidal breakup of…

星系天体物理 · 物理学 2015-06-11 Fupeng Zhang , Youjun Lu , Qingjuan Yu

Hypervelocity stars (HVSs) travel with velocities so extreme that dynamical ejection from a massive black hole is their only suggested origin. Following our discovery of the first HVS, we have undertaken a dedicated survey for more HVSs in…

天体物理学 · 物理学 2009-11-11 Warren R. Brown , Margaret J. Geller , Scott J. Kenyon , Michael J. Kurtz

Hypervelocity stars (HVS) move so fast that they are unbound to the Galaxy. When they were first discovered in 2005, dynamical ejection from the supermassive black hole (SMBH) in the Galactic Centre (GC) was suggested as their origin. The…

太阳与恒星天体物理 · 物理学 2015-04-15 E. Ziegerer , M. Volkert , U. Heber , A. Irrgang , B. T. Gaensicke , S. Geier

Hypervelocity stars (HVSs) discovered in the Milky Way (MW) halo are thought to be ejected from near the massive black hole (MBH) at the galactic centre. In this paper we investigate the spatial and velocity distributions of the HVSs which…

天体物理学 · 物理学 2009-11-13 Blake D. Sherwin , Abraham Loeb , Ryan M. O'Leary

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

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

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

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) 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

The last decade has seen the detection of fast moving stars in the Galactic halo, the so-called hypervelocity stars (HVSs). While the bulk of this population is likely the result of a close encounter between a stellar binary and the…

星系天体物理 · 物理学 2018-01-31 Giacomo Fragione , Alessia Gualandris
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