activity
20202022
most citedImplications of inhomogeneous metal mixing for stellar archaeology

32 citations · 67 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.IM202216 cited

A-SLOTH: Ancient Stars and Local Observables by Tracing Halos

Mattis Magg, Tilman Hartwig, Li-Hsin Chen +1

Galaxies are thought to reside inside of large gravitationally bound structures of dark matter, so-called haloes. While the smallest of these haloes host no or only a few stars, th…

astro-ph.GA202119 cited

Origin of metals in old Milky Way halo stars based on GALAH and Gaia

Miho N. Ishigaki, Tilman Hartwig, Yuta Tarumi +6

Stellar and supernova nucleosynthesis in the first few billion years of the cosmic history have set the scene for early structure formation in the Universe, while little is known a…

astro-ph.GA2021

Formation of an extended stellar halo around an ultra-faint dwarf galaxy following one of the earliest mergers from galactic building blocks

Yuta Tarumi, Naoki Yoshida, Anna Frebel

Ultra-faint dwarf galaxies (UFDs) are promising observable proxies to building blocks of galaxies formed in the early Universe. We study the formation and evolution of UFDs using c…

astro-ph.GA2021

Evidence for r-process delay in very metal-poor stars

Yuta Tarumi, Kenta Hotokezaka, Paz Beniamini

The abundances of r-process elements of very metal-poor stars capture the history of the r-process enrichment in the early stage of star formation in a galaxy. Currently, various t…

astro-ph.GA2021

-process enhancements of Gaia-Enceladus in GALAH DR3

Tadafumi Matsuno, Yutaka Hirai, Yuta Tarumi +3

The dominant site of production of -process elements remains unclear despite recent observations of a neutron star merger. Observational constraints on the properties of the sit…

astro-ph.GA202032 cited

Implications of inhomogeneous metal mixing for stellar archaeology

Yuta Tarumi, Tilman Hartwig, Mattis Magg

The first supernovae enrich the previously pristine gas with metals, out of which the next generation of stars form. Based on hydrodynamical simulations, we develop a new stochasti…