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相关论文: Systematic search for blue hyper-velocity stars fr…

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We report the discovery of 28 candidate high-velocity stars (HVSs) at heliocentric distances of less than 3 kpc, based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 1. Our sample of HVS candidates…

We describe a new survey for unbound hypervelocity stars (HVSs), stars traveling with such extreme velocities that dynamical ejection from a massive black hole (MBH) is their most likely origin. We investigate the possible contribution of…

天体物理学 · 物理学 2011-02-11 Warren R. Brown , Margaret J. Geller , Scott J. Kenyon

We report the first hypervelocity star (HVS) discovered from the LAMOST spectroscopic survey. It is a B-type star with a heliocentric radial velocity about 620 km/s, which projects to a Galactocentric radial velocity component of ~477 km/s.…

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…

We discuss our targeted search for hypervelocity stars (HVSs), stars traveling with velocities so extreme that dynamical ejection from a massive black hole is their only suggested origin. Our survey, now half complete, has successfully…

天体物理学 · 物理学 2008-11-26 Warren R. Brown , Margaret J. Geller , Scott J. Kenyon , Michael J. Kurtz

We present the discovery of five new unbound hypervelocity stars (HVSs) in the outer Milky Way halo. Using a conservative estimate of Galactic escape velocity, our targeted spectroscopic survey has now identified 16 unbound HVSs as well as…

星系天体物理 · 物理学 2015-06-04 Warren R. Brown , Margaret J. Geller , Scott J. Kenyon

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 report the discovery of two new unbound hypervelocity stars (HVSs) from the LAMOST spectroscopic surveys. They are respectively a B2V type star of ~ 7 M$_{\rm \odot}$ with a Galactic rest-frame radial velocity of 502 km/s at a…

星系天体物理 · 物理学 2017-10-04 Yang Huang , Xiaowei Liu , Huawei Zhang , Bingqiu Chen , Maosheng Xiang , Chun Wang , Haibo Yuan , Zhijia Tian , Yinbi Li , Bo Wang

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…

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

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 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 (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…

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

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

In this paper, we report the discovery of a new late-B type unbound hyper-runaway star (LAMOST-HVS4) from the LAMOST spectroscopic surveys. According to its atmospheric parameters, it is either a B-type main sequence (MS) star or a blue…

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 (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 describe our completed spectroscopic survey for unbound hypervelocity stars (HVSs) ejected from the Milky Way. Three new discoveries bring the total number of unbound HVSs to 21. We place new constraints on the nature of HVSs and on…

太阳与恒星天体物理 · 物理学 2015-06-18 Warren R. Brown , Margaret J. Geller , Scott J. Kenyon

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
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