The Pristine Inner Galaxy Survey (PIGS) – V. A chemo-dynamical investigation of the early assembly of the Milky Way with the most metal-poor stars in the bulge

Galaxy: evolution Galaxy evolution; globular clusters; stars-abundances stars: kinematics and dynamics FOS: Physical sciences stars: Population II Astrophysics - Astrophysics of Galaxies 01 natural sciences 520 Galaxy: bulge Astrophysics - Solar and Stellar Astrophysics [SDU]Sciences of the Universe [physics] Galaxy: formation 13. Climate action Astrophysics of Galaxies (astro-ph.GA) 0103 physical sciences Galaxy: abundances Solar and Stellar Astrophysics (astro-ph.SR)
DOI: 10.1093/mnras/stac3332 Publication Date: 2022-11-17T03:39:59Z
ABSTRACT
ABSTRACT The investigation of the metal-poor tail in Galactic bulge provides unique information on early Milky Way assembly and evolution. A chemo-dynamical analysis 17 very stars (VMP, [Fe/H]<−2.0) selected from Pristine Inner Galaxy Survey was carried out based Gemini/GRACES spectra. chemistry suggests that majority our are similar to halo. Orbits calculated Gaia EDR3 imply these brought into during earliest assembly. Most have large [Na,Ca/Mg] abundances, thus show little evidence enrichment by pair-instability supernovae. Two (P171457 P184700) chemical abundances compatible with second-generation globular cluster stars, suggestive presence ancient now dissolved clusters inner Galaxy. One them (P171457) is extremely ([Fe/H]<−3.0) well below metallicity floor clusters, which supports growing for existence lower-metallicity Universe. third star (P180956, [Fe/H]∼−2) has low [Ba/Fe] its metallicity, consistent formation a system polluted only one or few low-mass Interestingly, orbit confined plane, like other found literature, been associated building blocks Way.
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