Hypervelocity Stars. I. The Spectroscopic Survey
| dc.creator | Brown, Warren R. | |
| dc.creator | Geller, Margaret J. | |
| dc.creator | Kenyon, Scott J. | |
| dc.creator | Kurtz, Michael J. | |
| dc.date | 2006-04-05 | |
| dc.date | 2006-04-13 | |
| dc.date.accessioned | 2026-07-07T10:43:45Z | |
| dc.date.available | 2026-07-07T10:43:45Z | |
| dc.description | 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 identified a total of four probable HVSs plus a number of other unusual objects. Here we report the most recently discovered two HVSs: SDSS J110557.45+093439.5 and possibly SDSS J113312.12+010824, traveling with Galactic rest-frame velocities at least +508+-12 and +418+-10 km/s, respectively. The other late B-type objects in our survey are consistent with a population of post main-sequence stars or blue stragglers in the Galactic halo, with mean metallicity [Fe/H]=-1.3 and velocity dispersion 108+-5 km/s. Interestingly, the velocity distribution shows a tail of objects with large positive velocities that may be a mix of low-velocity HVSs and high-velocity runaway stars. Our survey also includes a number of DA white dwarfs with unusually red colors, possibly extremely low mass objects. Two of our objects are B supergiants in the Leo A dwarf, providing the first spectroscopic evidence for star formation in this dwarf galaxy within the last ~30 Myr. | |
| dc.description | 10 pages, uses emulateapj, accepted by ApJ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0604111 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0604111 | |
| dc.identifier | Astrophys.J.647:303-311,2006 | |
| dc.identifier | doi:10.1086/505165 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/182354 | |
| dc.subject | Astrophysics | |
| dc.title | Hypervelocity Stars. I. The Spectroscopic Survey | |
| dc.type | text |