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相关论文: Runaway M Dwarf Candidates from the Sloan Digital …

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We define an enhanced spectral classification scheme for M dwarf stars, and use it to derive spectral classification of 104 northern stars with proper motions larger than 0.5"/yr which we discovered in a survey of high proper motion stars…

天体物理学 · 物理学 2009-11-07 Sebastien Lepine , R. Michael Rich , Michael M. Shara

We present 20 candidate hypervelocity stars from the Sloan Extension for Galactic Understanding and Exploration (SEGUE) G and K dwarf samples. Previous searches for hypervelocity stars have only focused on large radial velocities; in this…

We measure the variation of the escape speed of the Galaxy across a range of $\sim$ 40 kpc in Galactocentric radius. The local escape speed is found to be $521^{+46}_{-30}\,\mathrm{km\,s^{-1}}$, in good agreement with other studies. We find…

星系天体物理 · 物理学 2017-04-19 Angus A. Williams , Vasily Belokurov , Andrew R. Casey , N. Wyn Evans

We present the results from a five-year campaign to gather multi-epoch, high-resolution spectra of a volume-complete sample of 413 M dwarfs with masses 10-30% that of the Sun that lie within 15 parsecs. We report weighted mean systemic…

Stars ejected from the Galactic centre can be used to place important constraints on the Milky Way potential. Since existing hypervelocity stars are too distant to accurately determine orbits, we have conducted a search for nearby…

星系天体物理 · 物理学 2016-12-06 Yanqiong Zhang , Martin C. Smith , Jeffrey L. Carlin

Hyper-velocity stars are believed to be ejected out from the Galactic center through dynamical interactions between (binary) stars and the central massive black hole(s). In this paper, we report 19 low mass F/G/K type hyper-velocity star…

Motivated by the historical identification of runaway main-sequence (MS) stars of early spectral type at high Galactic latitudes, we test the capability of Gaia at identifying new such stars. We have selected ~2300 sources with Gaia…

太阳与恒星天体物理 · 物理学 2024-09-05 Roberto Raddi , Andreas Irrgang , Ulrich Heber , David Schneider , Simon Kreuzer

Hypervelocity stars are believed to be ejected out from the Galactic center through dynamical interactions of (binary) stars with the central massive black hole(s). In this letter, we report 13 metal-poor F-type hypervelocity star…

太阳与恒星天体物理 · 物理学 2015-06-03 Yinbi Li , Ali Luo , Gang Zhao , Youjun Lu , Juanjuan Ren , Fang Zuo

As part of a radial velocity survey of low Galactic latitude structures that we undertook with the 2dF spectrograph on the AAT, we present the radial velocities of more than 1500 Red Giant Branch and Red Clump stars towards the centre of…

天体物理学 · 物理学 2009-11-10 N. F. Martin , R. A. Ibata , B. C. Conn , G. F. Lewis , M. Bellazzini , M. J. Irwin

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

(Abridged) We have obtained radial velocities of a sample of 18 ultracool dwarfs (M6.5-T8) using high-resolution, near-infrared spectra obtained with NIRSPEC and the Keck II telescope. We have confirmed that the radial velocity of Gl 570 D…

天体物理学 · 物理学 2009-06-23 M. R. Zapatero Osorio , E. L. Martin , V. J. S. Bejar , H. Bouy , R. Deshpande , R. J. Wainscoat

We report 23 stars having Galactocentric velocities larger than $450~\mathrm{km\,s}^{-1}$ in the final data release of the APOGEE survey. This sample was generated using space velocities derived by complementing the high quality radial…

According to LCDM theory, hierarchical evolution occurs on all mass scales, implying that satellites of the Milky Way should also have companions. The recent discovery of ultra-faint dwarf galaxy candidates in close proximity to the…

We present a new sample of M subdwarfs compiled from the 7th data release of the Sloan Digital Sky Survey. With 3517 new subdwarfs, this new sample significantly increases the number of spectroscopically confirmed low-mass subdwarfs. This…

太阳与恒星天体物理 · 物理学 2015-06-22 Antonia Savcheva , Andrew A. West , John J. Bochanski

Runaway stars ejected from the Galactic disk populate the halo of the Milky Way. To predict the spatial and kinematic properties of runaways, we inject stars into a Galactic potential, compute their trajectories through the Galaxy, and…

星系天体物理 · 物理学 2015-05-13 Benjamin C. Bromley , Scott J. Kenyon , Warren R. Brown , Margaret J. Geller

The dwarf carbon (dC) star SDSS J112801.67+004034.6 has an unusually high radial velocity, 531$\pm 4$ km s$^{-1}$. We present proper motion and new spectroscopic observations which imply a large Galactic rest frame velocity, 425$\pm 9$ km…

太阳与恒星天体物理 · 物理学 2016-12-28 Kathryn A. Plant , Bruce Margon , Puragra Guhathakurta , Emily C. Cunningham , Elisa Toloba , Jeffrey A. Munn

Hot subdwarfs (sdO/B) are the stripped helium cores of red giants formed by binary interactions. Close hot subdwarf binaries with massive white dwarf companions have been proposed as possible progenitors of thermonuclear supernovae type Ia…

We measure proper motions with the Hubble Space Telescope for 16 extreme radial velocity stars, mostly unbound B stars in the Milky Way halo. Twelve of these stars have proper motions statistically consistent with zero, and thus have radial…

太阳与恒星天体物理 · 物理学 2015-06-23 Warren R. Brown , Jay Anderson , Oleg Y. Gnedin , Howard E. Bond , Margaret J. Geller , Scott J. Kenyon

Distance estimates based on low-resolution spectroscopy and Two Micron All Sky Survey (2MASS) J magnitudes are presented for a large sample of 322 nearby candidates from Luyten's NLTT catalogue. Mainly relatively bright (typically 7 < K_s <…

天体物理学 · 物理学 2009-11-13 Ralf-Dieter Scholz , Helmut Meusinger , Hartmut Jahreiß

Runaway stars are OB-type stars ejected from their birthplace with large peculiar velocities. The leading hypothesis addressed in their formation includes the supernova ejection mechanism and the dynamic ejection scenario. Identification of…

太阳与恒星天体物理 · 物理学 2024-05-09 Yanjun Guo , Luqian Wang , Chao Liu , You Wu , ZhanWen Han , XueFei Chen
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