Evidence from APOGEE for the presence of a major building block of the halo buried in the inner Galaxy

Danny Horta, Ricardo P. Schiavon, J. Ted MacKereth, Joel Pfeffer, Andrew C. Mason, Shobhit Kisku, Francesca Fragkoudi, Carlos Allende Prieto, Katia Cunha, Sten Hasselquist, Jon Holtzman, Steven R. Majewski, David Nataf, Robert W. Oconnell, Mathias Schultheis, Verne V. Smith

Research output: Contribution to journalArticlepeer-review

26 Scopus citations

Abstract

We report evidence from APOGEE for the presence of a new metal-poor stellar structure located within ∼4 kpc of the Galactic Centre. Characterized by a chemical composition resembling those of low-mass satellites of the Milky Way, this new inner Galaxy structure (IGS) seems to be chemically and dynamically detached from more metal-rich populations in the inner Galaxy. We conjecture that this structure is associated with an accretion event that likely occurred in the early life of the Milky Way. Comparing the mean elemental abundances of this structure with predictions from cosmological numerical simulations, we estimate that the progenitor system had a stellar mass of ∼5 × 108 M, or approximately twice the mass of the recently discovered Gaia-Enceladus/Sausage system. We find that the accreted:in situ ratio within our metal-poor ([Fe/H] <-0.8) bulge sample is somewhere between 1:3 and 1:2, confirming predictions of cosmological numerical simulations by various groups.

Original languageEnglish (US)
Pages (from-to)1385-1403
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Volume500
Issue number1
DOIs
StatePublished - Jan 1 2021
Externally publishedYes

Keywords

  • Galaxy: Abundances
  • Galaxy: evolution
  • Galaxy: formation
  • Galaxy: halo
  • Galaxy: kinematics and dynamics
  • Galaxy: structure

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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