Identifying Sagittarius Stream Stars by Their APOGEE Chemical Abundance Signatures

Sten Hasselquist, Jeffrey L. Carlin, Jon A. Holtzman, Matthew Shetrone, Christian R. Hayes, Katia Cunha, Verne Smith, Rachael L. Beaton, Jennifer Sobeck, Carlos Allende Prieto, Steven R. Majewski, Borja Anguiano, Dmitry Bizyaev, D. A. Garca-Hernández, Richard R. Lane, Kaike Pan, David L. Nidever, José G. Fernández-Trincado, John C. Wilson, Olga Zamora

Research output: Contribution to journalArticlepeer-review

24 Scopus citations

Abstract

The SDSS-IV Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey provides precise chemical abundances of 18 chemical elements for ∼176,000 red giant stars distributed over much of the Milky Way Galaxy (MW), and includes observations of the core of the Sagittarius dwarf spheroidal galaxy (Sgr). The APOGEE chemical abundance patterns of Sgr have revealed that it is chemically distinct from the MW in most chemical elements. We employ a k-means clustering algorithm to six-dimensional chemical space defined by [(C+N)/Fe], [O/Fe], [Mg/Fe], [Al/Fe], [Mn/Fe], and [Ni/Fe] to identify 62 MW stars in the APOGEE sample that have Sgr-like chemical abundances. Of the 62 stars, 35 have Gaia kinematics and positions consistent with those predicted by N-body simulations of the Sgr stream, and are likely stars that have been stripped from Sgr during the last two pericenter passages (<2 Gyr ago). Another 20 of the 62 stars exhibit chemical abundances indistinguishable from the Sgr stream stars, but are on highly eccentric orbits with median r apo ∼ 25 kpc. These stars are likely the "accreted" halo population thought to be the result of a separate merger with the MW 8-11 Gyr ago. We also find one hypervelocity star candidate. We conclude that Sgr was enriched to [Fe/H] ∼ -0.2 before its most recent pericenter passage. If the "accreted halo" population is from one major accretion event, then this progenitor galaxy was enriched to at least [Fe/H] ∼ -0.6, and had a similar star formation history to Sgr before merging.

Original languageEnglish (US)
Article number58
JournalAstrophysical Journal
Volume872
Issue number1
DOIs
StatePublished - Feb 10 2019
Externally publishedYes

Keywords

  • galaxies: dwarf
  • galaxies: individual (Sagittarius dSph)
  • galaxies: stellar content

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Identifying Sagittarius Stream Stars by Their APOGEE Chemical Abundance Signatures'. Together they form a unique fingerprint.

Cite this