Takeru K. Suzuki

collaborators

4 papers

astro-ph.HE2025

Impacts of hydrogen envelope on supernova fallback and the resulting compact remnant masses

Kengo Shinoda, Yudai Suwa, Ryosuke Hirai +4

Fallback in core-collapse supernovae plays a central role in setting compact-remnant masses and may produce late-time emission. In hydrogen rich progenitors, the reverse shock aris…

astro-ph.SR2025

First VLBI Imaging of SiO $v = 0$ , $J = 1 \to 0$ Masers in VY Canis Majoris

Hiroko Shinnaga, Miyako Oyadomari, Hiroshi Imai +8

We achieved the first VLBI detections of the ground vibrational state ( $v = 0$ ) $^{28}$ SiO (hereafter, SiO) and $^{29}$ SiO masers of the $J = 1 \to 0$ rotational transitions, to…

astro-ph.SR2025

Red Giant Winds Driven by Alfvén Waves with Magnetic Diffusion

Takeru K. Suzuki, Keiichi Ohnaka, Yuki Yasuda

We investigate the driving mechanism of Alfvén wave-driven stellar winds from red giant stars, Arcturus ( $α$ Boo; K1.5 III) and Aldebaran ( $α$ Tau; K5 III), with nonideal MHD simul…

astro-ph.SR2024

Spin-down of solar-mass protostars in magnetospheric accretion paradigm

Shinsuke Takasao, Masanobu Kunitomo, Takeru K. Suzuki +2

Stellar spin is one of the fundamental quantities that characterize a star itself and its planetary system. Nevertheless, stellar spin-down mechanisms in protostellar and pre-main-…

Impacts of hydrogen envelope on supernova fallback and the resulting compact remnant masses

First VLBI Imaging of SiO v=0, J=1→0 Masers in VY Canis Majoris

Red Giant Winds Driven by Alfvén Waves with Magnetic Diffusion

Spin-down of solar-mass protostars in magnetospheric accretion paradigm

First VLBI Imaging of SiO $v = 0$ , $J = 1 \to 0$ Masers in VY Canis Majoris