Abundance Patterns of and Neutron-capture Elements in the Helmi Stream
arXiv:2105.05958 · doi:10.3847/2041-8213/ac0056
Abstract
We identified 8 additional stars as members of the Helmi stream (HStr) in the combined GALAH+ DR3 and EDR3 catalog. By consistently reevaluating claimed members from the literature, we consolidate a sample of 22 HStr stars with parameters determined from high-resolution spectroscopy and spanning a considerably wider (by 0.5 dex) metallicity interval () than previously reported. Our study focuses on (Mg and Ca) and neutron-capture (Ba and Eu) elements. We find that the chemistry of HStr is typical of dwarf spheroidal (dSph) galaxies, in good agreement with previous -body simulations of this merging event. Stars of HStr constitute a clear declining sequence in for increasing metallicity up to . Moreover, stars of HStr show a median value of 0.5 dex for with a small dispersion (0.1 dex). Every star analyzed with belong to the -process enhanced ( and ) metal-poor category, providing remarkable evidence that, at such low-metallicity regime, stars of HStr experienced enrichment in neutron-capture elements predominantly via -process nucleosynthesis. Finally, the extended metallicity range also suggests an increase in for higher , in conformity with other surviving dwarf satellite galaxies of the Milky Way.
arXiv comment9 pages (+2 appendix), 4 figures. Accepted for publication in ApJ Letters
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