APOGEE-2 Discovery of a Large Population of Relatively High-Metallicity Globular Cluster Debris
arXiv:2109.02669 · doi:10.3847/2041-8213/ac225b
Abstract
We report the discovery of a new, chemically distinct population of relatively high-metallicity ([Fe/H] ) red giant stars with super-solar [N/Fe] () identified within the bulge, disk, and halo of the Milky Way. This sample of stars was observed during the second phase of the Apache Point Observatory Galactic Evolution Experiment (APOGEE-2); the spectra of these stars are part of the seventeenth Data Release (DR 17) of the Sloan Digital Sky Survey. We hypothesize that this newly identified population was formed in a variety of progenitors, and are likely made up of either fully or partially destroyed metal-rich globular clusters, which we refer to as Globular Cluster Debris (GCD), identified by their unusual photospheric nitrogen abundances. It is likely that some of the GCD stars were probable members of the Gaia-Enceladus-Sausage accretion event, along with clusters formed in situ.
arXiv comment9 pages, 4 figures, 1 table, accepted for publication in The Astrophysical Journal Letters
References in corpus (39)
- The 2.5 m Telescope of the Sloan Digital Sky Survey
- The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
- Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
- Co-formation of the Galactic disc and the stellar halo
- ASPCAP: The Apogee Stellar Parameter and Chemical Abundances Pipeline
- Gaia Data Release 2: Kinematics of globular clusters and dwarf galaxies around the Milky Way
- Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
- Gaia EDR3 view on Galactic globular clusters
- The Data Reduction Pipeline for the Apache Point Observatory Galactic Evolution Experiment
- Origin of the system of globular clusters in the Milky Way
- Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST and literature data
- The Apache Point Observatory Galactic Evolution Experiment (APOGEE) Spectrographs
- Target Selection for the SDSS-IV APOGEE-2 Survey
- APOGEE Data Releases 13 and 14: Data and Analysis
- -process production in rotating massive stars at solar and low metallicities
- StarHorse: A Bayesian tool for determining stellar masses, ages, distances, and extinctions for field stars
- Chemical tagging with APOGEE: Discovery of a large population of N-rich stars in the inner Galaxy
- From the bulge to the outer disc: StarHorse stellar parameters, distances, and extinctions for stars in APOGEE DR16 and other spectroscopic surveys
- The SDSS-III APOGEE Spectral Line List for H-band Spectroscopy
- Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code. II. The Southern Clusters and Overview
- The APOGEE Data Release 16 Spectral Line List
- The pattern speed of the Milky Way bar from transverse velocities
- New H-band Stellar Spectral Libraries for the SDSS-III/APOGEE survey
- Chemical tagging in the SDSS-III/APOGEE survey: new identifications of halo stars with globular cluster origins
- Atypical Mg-poor Milky Way field stars with globular cluster second-generation like chemical patterns
- Constraining Metallicity-dependent Mixing and Extra Mixing using [C/N] in Alpha-Rich Field Giants
- The ASAS-SN Catalog of Variable Stars IX: The Spectroscopic Properties of Galactic Variable Stars
- Discovery of a Metal-Poor Field Giant with a Globular Cluster Second-Generation Abundance Pattern
- The tidal remnant of an unusually metal-poor globular cluster
- Chemodynamics of newly identified giants with globular cluster like abundance patterns in the bulge, disk, and halo of the Milky Way
- Aluminum Enhanced Metal-Poor Stars buried in the Inner Galaxy
- Discovery of a new stellar sub-population residing in the (inner) stellar halo of the Milky Way
- Dynamical Orbital classification of selected N-rich stars with \textit{Gaia} DR2 astrometry
- Purveyors of fine halos. II. Chemodynamical association of halo stars with Milky Way globular clusters
- Chemical analysis of CH stars - II: atmospheric parameters and elemental abundances
- VVV CL001: Likely the Most Metal-Poor Surviving Globular Cluster in the Inner Galaxy
- Jurassic: A Chemically Anomalous Structure in the Galactic Halo
- Discovery of a large population of Nitrogen-Enhanced stars in the Magellanic Clouds
- The most metal-poor Galactic globular cluster: the first spectroscopic observations of ESO280-SC06
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- Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO) I. An updated census of APOGEE N-rich giants across the Milky Way
- Orbits of globular clusters computed with dynamical friction in the Galactic anisotropic velocity dispersion field
- Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO) II. t-SNE Portrait of Local Fossil Relics and Structures
- Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal) II. Unveiling the formation and evolution of the kinematically selected Thick and Thin Discs
- Determination of Sodium Abundance Ratio from Low-Resolution Stellar Spectra and Its Applications