Hypervelocity stars
WR Brown - Annual Review of Astronomy and Astrophysics, 2015 - annualreviews.org
Hypervelocity stars (HVSs) travel with such extreme velocities that dynamical ejection via
gravitational interaction with a massive black hole (MBH) is their most likely origin …
gravitational interaction with a massive black hole (MBH) is their most likely origin …
The RAVE survey: the Galactic escape speed and the mass of the Milky Way
T Piffl, C Scannapieco, J Binney, M Steinmetz… - Astronomy & …, 2014 - aanda.org
We made new estimates of the Galactic escape speed at various Galactocentric radii using
the latest data release of the RAdial Velocity Experiment (RAVE DR4). Compared to …
the latest data release of the RAdial Velocity Experiment (RAVE DR4). Compared to …
Dwarf galaxy planes: the discovery of symmetric structures in the Local Group
MS Pawlowski, P Kroupa… - Monthly Notices of the …, 2013 - academic.oup.com
Both major galaxies in the Local Group (LG) are surrounded by thin planes of mostly co-
orbiting satellite galaxies, the vast polar structure (VPOS) around the Milky Way (MW) and …
orbiting satellite galaxies, the vast polar structure (VPOS) around the Milky Way (MW) and …
MMT hypervelocity star survey. III. The complete survey
WR Brown, MJ Geller, SJ Kenyon - The Astrophysical Journal, 2014 - iopscience.iop.org
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 late B …
ejected from the Milky Way. Three new discoveries bring the total number of unbound late B …
Hyper-runaway and hypervelocity white dwarf candidates in Gaia Data Release 3: Possible remnants from Ia/Iax supernova explosions or dynamical encounters
AP Igoshev, H Perets… - Monthly Notices of the …, 2023 - academic.oup.com
Type Ia and other peculiar supernovae (SNe) are thought to originate from the
thermonuclear explosions of white dwarfs (WDs). Some of the proposed channels involve …
thermonuclear explosions of white dwarfs (WDs). Some of the proposed channels involve …
Identifying sagittarius stream stars by their APOGEE chemical abundance signatures
S Hasselquist, JL Carlin, JA Holtzman… - The Astrophysical …, 2019 - iopscience.iop.org
Abstract The SDSS-IV Apache Point Observatory Galactic Evolution Experiment (APOGEE)
survey provides precise chemical abundances of 18 chemical elements for∼ 176,000 red …
survey provides precise chemical abundances of 18 chemical elements for∼ 176,000 red …
Proper Motions and Trajectories for 16 Extreme Runaway and Hypervelocity Stars
WR Brown, J Anderson, OY Gnedin… - The Astrophysical …, 2015 - iopscience.iop.org
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 …
stars, mostly unbound B stars in the Milky Way halo. Twelve of these stars have proper …
Mmt hypervelocity star survey. ii. Five new unbound stars
WR Brown, MJ Geller, SJ Kenyon - The Astrophysical Journal, 2012 - iopscience.iop.org
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 …
Way halo. Using a conservative estimate of Galactic escape velocity, our targeted …
On the Origins of Extreme Velocity Stars as Revealed by Large-scale Galactic Surveys
QZ Li, Y Huang, XB Dong, HW Zhang… - The Astronomical …, 2023 - iopscience.iop.org
We assemble a large sample of 12,784 high-velocity stars with total velocity V GSR≥ 300
km s− 1, selected from RAVE DR5, SDSS DR12, LAMOST DR8, APOGEE DR16, GALAH …
km s− 1, selected from RAVE DR5, SDSS DR12, LAMOST DR8, APOGEE DR16, GALAH …
Discovery of a Hypervelocity L Subdwarf at the Star/Brown Dwarf Mass Limit
We report the discovery of a high-velocity, very low-mass star or brown dwarf whose
kinematics suggest it is unbound to the Milky Way. CWISE J124909. 08+ 362116.0 was …
kinematics suggest it is unbound to the Milky Way. CWISE J124909. 08+ 362116.0 was …