activity
19962023
most citedGalactic chemical evolution: Carbon through Zinc

890 citations · 17.4k across the 216 of their papers we have counts for

collaborators

217 papers

astro-ph.HE2023★ 11 cited

Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae I: Parameter Study of the Dependence on Jet Energetics

Shing-Chi Leung, Ken'ichi Nomoto, Tomoharu Suzuki

Rotating massive stars with initial progenitor masses 25 -- 140 can leave rapidly rotating black holes to become collapsars. The b…

astro-ph.HE2023★ 9 cited

Ambipolar Heating of Magnetars

Sachiko Tsuruta, Madeline J. Kelly, Ken'ichi Nomoto +3

Magnetars, neutron stars thought to be with ultra-strong magnetic fields of G, are observed to be much hotter than ordinary pulsars with G, and additi…

astro-ph.HE2022★ 15 cited

The Late-Time Light Curves of Type Ia Supernovae: Confronting Models with Observations

Vishal Tiwari, Or Graur, Robert Fisher +5

Type Ia supernovae (SNe Ia) play a crucial role as standardizable candles in measurements of the Hubble constant and dark energy. Increasing evidence points towards multiple possib…

astro-ph.HE2021★ 25 cited

Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence

Shuai Zha, Evan P. O'Connor, Sean M. Couch +2

We present neutrino-transport hydrodynamic simulations of electron-capture supernovae (ECSNe) in \texttt{FLASH} with new two-dimensional (2D) collapsing progenitor models. These pr…

astro-ph.HE2021★ 3 cited

Type Ia Supernovae and their Explosive Nucleosynthesis: Constraints on Progenitors

Shing-Chi Leung, Ken'ichi Nomoto

What the progenitors of Type Ia supernovae (SNe Ia) are, whether they are near-Chandrasekhar mass or sub-Chandrasekhar mass white dwarfs, has been the matter of debate for decades.…

astro-ph.HE2021★ 11 cited

Spatially Resolved X-ray Study of Supernova Remnant G306.30.9 with Unusually High Calcium Abundance

Jianbin Weng, Ping Zhou, Yang Chen +6

G306.30.9 is an asymmetric Galactic supernova remnant (SNR), whose progenitor has been thought to be a Type Ia supernova (SN), but its high Ca abundance appears inconsistent wit…