most citedEarly chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements

40 citations · 63 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20232 cited

Surrogate Modeling for Computationally Expensive Simulations of Supernovae in High-Resolution Galaxy Simulations

Keiya Hirashima, Kana Moriwaki, Michiko S. Fujii +4

Some stars are known to explode at the end of their lives, called supernovae (SNe). The substantial amount of matter and energy that SNe release provides significant feedback to st…

astro-ph.GA20232 cited

Probing the Galactic Halo with RR Lyrae Stars -- V. Chemistry, Kinematics, and Dynamically Tagged Groups

Jonathan Cabrera Garcia, Timothy C. Beers, Yang Huang +9

We employ a sample of 135,873 RR Lyrae stars (RRLs) with precise photometric-metallicity and distance estimates from the newly calibrated ------[Fe/H] and

astro-ph.GA202317 cited

Insights on the Sun birth environment in the context of star-cluster formation in hub-filament systems

Doris Arzoumanian, Sota Arakawa, Masato I. N. Kobayashi +7

Cylindrical molecular filaments are observed to be the main sites of Sun-like star formation, while massive stars form in dense hubs, at the junction of multiple filaments. The rol…

astro-ph.GA20232 cited

The Origin of the Large Magellanic Cloud Globular Cluster NGC 2005

Andrés E. Piatti, Yutaka Hirai

The ancient Large Magellanic Cloud (LMC) globular cluster NGC 2005 has recently been reported to have an ex-situ origin, thus, setting precedents that the LMC could have partially…

astro-ph.GA201640 cited

Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements

Yutaka Hirai, Yuhri Ishimaru, Takayuki R. Saitoh +3

The abundance of elements synthesized by the rapid neutron-capture process (r-process elements) of extremely metal-poor (EMP) stars in the Local Group galaxies gives us clues to cl…