Issue |
EAS Publications Series
Volume 67-68, 2014
The Milky Way Unravelled by Gaia: GREAT Science from the Gaia Data Releases
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Page(s) | 255 - 259 | |
Section | The Origin and History of the Milky Way | |
DOI | https://doi.org/10.1051/eas/1567046 | |
Published online | 17 July 2015 |
N.A. Walton, F. Figueras, L. Balaguer-Núñez and C. Soubiran (eds)
EAS Publications Series, 67–68 (2014) 255-259
Nearby Low-Mass Hypervelocity Stars
1 Shanghai Astronomical Observatory
2 Rensselaer Polytechnic Institute, Troy & Earlham College, Richmond, USA
e-mail: zhangyq@shao.ac.cn
e-mail: msmith@shao.ac.cn
Hypervelocity stars are those that have speeds exceeding the escape speed and are hence unbound from the Milky Way. We investigate a sample of low-mass hypervelocity candidates obtained using data from the high-precision SDSS Stripe 82 catalogue, which we have combined with spectroscopy from the 200-inch Hale Telescope at Palomar Observatory. We find four good candidates, but without metallicities it is difficult to pin-down their distances and therefore total velocities. Our best candidate has a significant likelihood that it is escaping the Milky Way for a wide-range of metallicities.
© EAS, EDP Sciences, 2015