Hypervelocity Stars Track Back to the Galactic Center in Gaia DR3

Based on the proper motions and radial velocities from Gaia Data Release 3, we identify two hypervelocity stars (HVSs) that may originate from the Galactic center (GC). We select the candidates by first filtering for all Gaia stars with Galactocentric radial velocities >500 km s −1 . We also requ...

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Bibliographic Details
Published inAstrophysical journal. Letters Vol. 944; no. 2; p. L39
Main Authors Liao, Jiwei, Du, Cuihua, Li, Hefan, Ma, Jun, Shi, Jianrong
Format Journal Article
LanguageEnglish
Published Austin The American Astronomical Society 01.02.2023
IOP Publishing
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