21 citations · 32 across the 3 of their papers we have counts for
4 papers
Are Faint Supernovae Responsible for Carbon-Enhanced Metal-Poor Stars?
Yutaka Komiya, Takuma Suda, Shimako Yamada +1
Mixing and fallback models in faint supernova models are supposed to reproduce the abundance patterns of observed carbon-enhanced metal-poor (CEMP) stars in the Galactic halo. A fi…
R-process Element Cosmic Rays from Neutron Star Mergers
Yutaka Komiya, Toshikazu Shigeyama
Neutron star mergers (NSMs) are one of the most plausible sources of r-process elements in the universe. Therefore NSMs can also be a major source of ultra-heavy elements in cosmic…
Population III stars around the Milky Way
Yutaka Komiya, Takuma Suda, Masayuki Y. Fujimoto
We explore the possibility of observing Population III (Pop~III) stars, born of the primordial gas. Pop~III stars with masses below should survive to date though are…
Prototype Implementation of Web and Desktop Applications for ALMA Science Verification Data and the Lessons Learned
Satoshi Eguchi, Wataru Kawasaki, Yuji Shirasaki +4
ALMA is estimated to generate TB scale data during only one observation; astronomers manage to identify which part of the data they are really interested in. Now we have been devel…