Proper Motions and Trajectories for 16 Extreme Runaway and Hypervelocity Stars
arXiv:1502.05069 · doi:10.1088/0004-637X/804/1/49
Abstract
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 trajectories statistically consistent with a Galactic center "hypervelocity star" origin. The trajectory of HE 0437-5439 is consistent with both Milky Way and Large Magellanic Cloud origins. A Galactic center origin is excluded at 3-sigma confidence for two of the lowest radial velocity stars in our sample, however. These two stars are probable disk runaways and provide evidence for ~500 km/s ejections from the disk. We also measure a significant proper motion for the unbound sdO star US 708. Its 1,000 km/s motion is in some tension with proposed supernova ejection models, but can be explained if US 708 was ejected from the stellar halo. In the future, we expect Gaia will better constrain the origin of these remarkable unbound stars.
11 pages, 5 figures, submitted to ApJ
References in corpus (16)
- Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. I. Sample Selection, Data Reduction and NGC 7078 Results
- Hypervelocity Stars. I. The Spectroscopic Survey
- An Alternative Origin for Hypervelocity Stars
- On type Ia supernovae and the formation of single low-mass white dwarfs
- Hypervelocity Stars: From the Galactic Center to the Halo
- A Successful Targeted Search for Hypervelocity Stars
- Maximum speed of hypervelocity stars ejected from binaries
- Hypervelocity Stars III. The Space Density and Ejection History of Main Sequence Stars from the Galactic Center
- Runaway and hypervelocity stars in the Galactic halo: Binary rejuvenation and triple disruption
- Predicted Space Motions for Hypervelocity and Runaway Stars: Proper Motions and Radial Velocities for the GAIA Era
- LMC origin of the hyper-velocity star HE 0437-5439. Beyond the supermassive black hole paradigm
- The Nature of the Hyper-Runaway Candidate HIP 60350
- A Galactic Center Origin for HE 0437-5439, the Hypervelocity Star near the Large Magellanic Cloud
- HVS7: a chemically peculiar hyper-velocity star
- Low Metallicity Indicates that the Hypervelocity Star HE 0437-5439 was Ejected from the LMC
- 'Slow' and Fast Rotators among Hypervelocity Stars
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- Gaia DR3 in 6D: The search for fast hypervelocity stars and constraints on the Galactic Centre environment
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- Faint objects in motion: the new frontier of high precision astrometry
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- An artificial neural network to discover Hypervelocity stars: Candidates in Gaia DR1/TGAS
- Masses of White Dwarf Binary Companions to Type Ia Supernovae Measured from Runaway Velocities
- Hypervelocity Stars in the Gaia era. Revisiting the most extreme stars from the MMT survey
- Tidal breakup of triple stars in the Galactic Centre
- Milky Way archaeology using RR Lyrae and type II Cepheids II. High velocity RR Lyrae stars, and mass of the Milky Way
- Mergers of Equal-Mass Binaries with Compact Object Companions from Mass Transfer in Triple Star Systems
- Constraints on the Galactic Centre environment from Gaia hypervelocity stars II: The evolved population
- Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
- Candidate Hypervelocity Red Clump Stars in the Galactic Bulge Found Using the VVV and Gaia Surveys
- Harnessing the Hubble Space Telescope Archives: A Catalogue of 21,926 Interacting Galaxies
- Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars
- Discovery of Galactic center ejected star in DESI DR1
- The Fate of Binary Stars Hosting Planets upon Interaction with Sgr A* Black hole
- Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae
- An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing