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相关论文: Where are the Old-Population High Velocity Stars?

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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 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

We present limits on the ejection of old-population HVS from a sample of over 290,000 stars selected from the SDSS. We derive the speed at the solar circle from the measured positions and radial velocities by assuming a radial orbit and…

天体物理学 · 物理学 2015-05-13 Juna A. Kollmeier , Andrew Gould , Gillian Knapp , Timothy C. Beers

We report the discovery of 3 new unbound hypervelocity stars (HVSs), stars traveling with such extreme velocities that dynamical ejection from a massive black hole (MBH) is their only suggested origin. We also detect a population of…

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

We search for high-velocity stars in the inner region of the Galactic bulge using a selected sample of red clump stars. Some of those stars might be considered hypervelocity stars (HVSs). Even though the HVSs ejection relies on an…

We report the results of a photometric search for giant stars associated with the cores of four high velocity clouds (HVCs) -- two of which are compact HVCs -- using the Las Campanas Du Pont 2.5 meter and Cerro Tololo Blanco 4 meter…

天体物理学 · 物理学 2009-11-10 M. H. Siegel , S. R. Majewski , C. Gallart , S. Sohn , W. E. Kunkel , R. Braun

We have computed the galactic trajectories of twelve hypervelocity stars (HVSs) under the assumption that they originated in the Galactic Centre. We show that eight of these twelve stars are bound to the Galaxy. We consider the subsequent…

天体物理学 · 物理学 2009-11-13 Karl M. Svensson , Ross P. Church , Melvyn B. Davies

In recent years several hypervelocity stars (HVSs) have been observed in the halo of our Galaxy. Such HVSs have possibly been ejected from the Galactic center and then propagated in the Galactic potential up to their current position. The…

天体物理学 · 物理学 2011-02-11 Hagai B. Perets , Xufen Wu , HongSheng Zhao , Benoit Famaey , Gianfranco Gentile , Tal Alexander

Hypervelocity stars (HVSs) represent a unique class of objects capable of escaping the gravitational pull of the Milky Way due to extreme acceleration events, such as close encounters with the supermassive black hole at the Galactic center…

星系天体物理 · 物理学 2025-04-22 Yongkang Sun , Yang Huang , Jifeng Liu , Haozhu Fu , Huawei Zhang , Yinbi Li , Cuihua Du , Jianrong Shi , Xiao Kong

The first three hyper-velocity stars (HVS) unbound to the Galaxy were serendipitously discovered in 2005. The only suggested origin of hyper-velocity stars is the Galactic Centre as it hosts a super-massive black hole capable of…

天体物理学 · 物理学 2008-05-08 Uli Heber , Heiko Hirsch , Heinz Edelmann , Ralf Napiwotzki , Simon O`Toole , Warren Brown , Martin Altmann

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 (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

We assemble a large sample of 12,784 high-velocity stars with total velocity $\it{V}_{\rm{GSR}}\ge {\rm 300}$ km s$^{-1}$, selected from RAVE DR5, SDSS DR12, LAMOST DR8, APOGEE DR16, GALAH DR2, and $Gaia$ EDR3. In this sample, 52 are…

星系天体物理 · 物理学 2023-06-28 Qing-Zheng Li , Yang Huang , Xiao-Bo Dong , Hua-Wei Zhang , Timothy C. Beers , Zhen Yuan

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

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

Hypervelocity stars (HVSs) escaping away from the Galactic halo are dynamical products of interactions of stars with the massive black hole(s) (MBH) in the Galactic Center (GC). They are mainly B-type stars with their progenitors unknown.…

星系天体物理 · 物理学 2011-05-13 Youjun Lu , Fupeng Zhang , Qingjuan Yu

Hypervelocity stars (HVSs) are stars which have been ejected from the Galactic Centre (GC) at velocities of up to a few thousand km/s. They are tracers of the Galactic potential and can be used to infer properties of the GC, such as the…

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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