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
AUTHORS (16)
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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