Lessons from the curious case of the `fastest' star in Gaia DR2

Douglas Boubert, Jay Strader, David Aguado, George Seabroke, Sergey Koposov, Jason Sanders, Samuel Swihart, Laura Chomiuk, N. Wyn Evans

Research output: Contribution to journalArticlepeer-review

Abstract

Gaia DR2 5932173855446728064 was recently proposed to be unbound from the Milky Way based on the −614.3±2.5kms−1 median radial velocity given in Gaia DR2. We obtained eight epochs of spectroscopic follow-up and find a very different median radial velocity of −56.5±5.3kms−1⁠. If this difference were to be explained by binarity, then the unseen companion would be an intermediate-mass black hole; we therefore argue that the Gaia DR2 radial velocity must be in error. We find it likely that the spectra obtained by Gaia were dominated by the light from a star 4.3arcsec away, and that, due to the slitless, time delay integration nature of Gaia spectroscopy, this angular offset corresponded to a spurious 620kms−1 shift in the calcium triplet of the second star. We argue that such unanticipated alignments between stars may account for 105 of the 202 stars with radial velocities faster than 500kms−1 in Gaia DR2 and propose a quality cut to exclude stars that are susceptible. We propose further cuts to remove stars where the colour photometry is suspect and stars where the radial velocity measurement is based on fewer than four transits, and thus produce an unprecedentedly clean selection of Gaia radial velocities for use in studies of Galactic dynamics.
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Early online date29 Jan 2019
DOIs
Publication statusPublished - 1 Jun 2019

Keywords

  • astro-ph.SR
  • astro-ph.GA

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