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20142025
most citedPopulation Studies. XIII. A New Analysis of the Bidelman-MacConnell "Weak-Metal" Stars - Confirmation of Metal-Poor Stars in the Thick Disk of the Galaxy

91 citations · 693 across the 20 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.GA2022★ 26 cited

Phase-space Properties and Chemistry of the Sagittarius Stellar Stream Down to the Extremely Metal-poor () Regime

Guilherme Limberg, Anna B. A. Queiroz, Hélio D. Perottoni +6

In this work, we study the phase-space and chemical properties of Sagittarius (Sgr) stream, the tidal tails produced by the ongoing destruction of Sgr dwarf spheroidal (dSph) galax…

astro-ph.GA2022★ 13 cited

Chemodynamical Analysis of Metal-rich High-eccentricity Stars in the Milky Way's Disk

Ayeon Lee, Young Sun Lee, Young Kwang Kim +2

We present a chemodynamical analysis of 11,562 metal-rich, high-eccentricity halo-like main-sequence (MS) stars, which has been referred to as the Splash or Splashed Disk, selected…

astro-ph.SR2022★ 20 cited

Mining S-PLUS for Metal-Poor Stars in the Milky Way

Vinicius M. Placco, Felipe Almeida-Fernandes, Anke Arentsen +4

This work presents the medium-resolution () spectroscopic follow-up of 522 low-metallicity star candidates from the Southern Photometric Local Universe Survey (S-PLUS…

astro-ph.GA2022★ 28 cited

Carbon-Enhanced Metal-Poor star candidates from BP/RP Spectra in DR3

Madeline Lucey, Nariman Al Kharusi, Keith Hawkins +6

Carbon-enhanced metal-poor (CEMP) stars comprise almost a third of stars with [Fe/H] < --2, although their origins are still poorly understood. It is highly likely that one sub-cla…

astro-ph.GA2022★ 40 cited

On the inconsistency of [C/Fe] abundances and the fractions of carbon-enhanced metal-poor stars among various stellar surveys

Anke Arentsen, Vinicius M. Placco, Young Sun Lee +4

Carbon-enhanced metal-poor (CEMP) stars are a unique resource for Galactic archaeology because they probe the properties of the First Stars, early chemical evolution and binary int…