University of Hertfordshire

From the same journal

From the same journal

By the same authors

Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys

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  • 2011.08305

    Accepted author manuscript, 7.03 MB, PDF document

  • Guilherme Limberg
  • Silvia Rossi
  • Timothy Beers
  • Helio Perottoni
  • Angeles Perez-Villegas
  • Rafael Santucci
  • Yuri Abuchaim
  • Vinicius Placco
  • Young Sun Lee
  • Norbert Christlieb
  • John Norris
  • Michael Bessell
  • Sean Ryan
  • Ronald Wilhelm
  • Jaehyon Rhee
  • Anna Frebel
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Original languageEnglish
Article number10
Number of pages25
JournalThe Astrophysical Journal
Volume907
Issue1
DOIs
Publication statusPublished - 20 Jan 2021

Abstract

We analyze the dynamical properties of ∼1500 very metal-poor (VMP; [Fe/H] ≲−2.0) halo stars, based primarily on medium-resolution spectroscopic data from the HK and Hamburg/ESO surveys. These data, collected over the past thirty years, are supplemented by a number of calibration stars and other small samples, along with astrometric information from Gaia DR2. We apply a clustering algorithm to the 4-D energy-action space of the sample, and identify a set of 38 Dynamically Tagged Groups (DTGs), containing between 5 and 30 member stars. Many of these DTGs can be associated with previously known prominent substructures such as Gaia-Sausage/Enceladus (GSE), Sequoia, the Helmi Stream (HStr), and Thamnos. Others are associated with previously identified smaller dynamical groups of stars and streams. We identify 10 new DTGs as well, many of which have strongly retrograde orbits. We also investigate possible connections between our DTGs and ∼300 individual r-process-enhanced (RPE) stars \textbf{from a recent literature compilation}. We find that several of these objects have similar dynamical properties to GSE (5), the HStr (4), Sequoia (1), and Rg5 (1), indicating that their progenitors might have been important sources of RPE stars in the Galaxy. Additionally, a number of our newly identified DTGs are shown to be associated with at least two RPE stars each (DTG-2: 3, DTG-7: 2; DTG-27: 2). Taken as a whole, these results are consistent with ultra-faint and/or dwarf spheroidal galaxies as birth environments in which r-process nucleosynthesis took place, and then were disrupted by the Milky Way.

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