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An Old, Low-mass, Metal-poor Hypervelocity Star Candidate Consistent with a Galactic Center Origin

The Astrophysical Journal Letters, vol. 1003, pp. L9

Abstract

Abstract We report the discovery of DESI-HVS1, a hypervelocity star (HVS) candidate identified from DESI DR1 spectroscopy and Gaia DR3 astrometry. DESI-HVS1 is an old, low-mass, metal-poor F-type star with a mass of 0.8 M ⊙ , an age of ∼14.1 Gyr, and [Fe/H] = −1.6. It is located at a heliocentric distance of 3.7 7 − 0.36 + 0.39 kpc and has a Galactocentric total velocity of 52 3 − 47 + 46 km s − 1 , marginally exceeding the local escape speed, corresponding to an unbound probability of P ub ∼ 50%. Backward orbit integrations show that DESI-HVS1 had the closest approach to the Galactic center (GC) of 0.4 0 − 0.11 + 0.23 kpc , with a velocity of 68 2 − 35 + 22 km s − 1 and a flight time of 12.8 9 − 0.74 + 0.92 Myr . The reconstructed orbit exhibits a clear perigalactic turning point and only a single crossing of the Galactic midplane ( P cross > 0.95). These properties suggest that DESI-HVS1 is most naturally explained by the Hills mechanism, although alternative scenarios cannot be entirely ruled out. Its discovery provides the first strong evidence for an old, low-mass HVS candidate consistent with a GC origin, indicating that the apparent dominance of young, massive GC-origin HVSs is likely a consequence of observational selection effects.

Authors 7

  1. China West Normal University · University of Chinese Academy of Sciences

    Affiliation as printed

    China West Normal University

    University of Chinese Academy of Sciences

  2. Chinese Academy of Sciences · University of Chinese Academy of Sciences

    Affiliation as printed

    Chinese Academy of Sciences

    University of Chinese Academy of Sciences

  3. Peking University

    Affiliation as printed

    Peking University

  4. Chinese Academy of Sciences · University of Chinese Academy of Sciences

    Affiliation as printed

    Chinese Academy of Sciences

    University of Chinese Academy of Sciences

  5. Peking University

    Affiliation as printed

    Peking University

  6. Guoyang Chen Aachen

    Leiden University · Chinese Academy of Sciences

    Affiliation as printed

    Chinese Academy of Sciences

    Leiden University

  7. Peking University

    Affiliation as printed

    Peking University

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References 51