activity
20142024
most citedSpiral Structure and Differential Dust Size Distribution in the LkHa 330 Disk

35 citations · 159 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP20242 cited

Predicting the Dominant Formation Mechanism of Multi-Planetary Systems

Cheyanne Shariat, Yasuhiro Hasegawa, Bradley M. S. Hansen +2

Most, if not all, sun-like stars host one or more planets, making multi-planetary systems commonplace in our galaxy. We utilize hundreds of multi-planet simulations to explore the…

astro-ph.EP2024

Forming localized dust concentrations in a dust ring: DM Tau case study

Hauyu Baobab Liu, Takayuki Muto, Mihoko Konishi +8

The previous, high angular resolution 225 GHz (1.3 mm) continuum observations on the transitional disk DM Tau have resolved an outer ring at 20-120 au radii that is weakly az…

astro-ph.EP2024

Testing magnetospheric accretion as an H emission mechanism of embedded giant planets: The case study for the disk exhibiting meridional flow around HD 163296

Yasuhiro Hasegawa, Taichi Uyama, Jun Hashimoto +7

Recent high-sensitivity observations reveal that accreting giant planets embedded in their parental circumstellar disks can emit H at their final formation stages. While the ori…

astro-ph.EP2023

A Primordial Origin for the Gas-Rich Debris Disks Around Intermediate-Mass Stars

Riouhei Nakatani, Neal J. Turner, Yasuhiro Hasegawa +4

While most debris disks consist of dust with little or no gas, a fraction has significant amounts of gas detected via emission lines of CO, ionized carbon, and/or atomic oxygen. Al…

astro-ph.IM202311 cited

PRIMA General Observer Science Book

A. Moullet, T. Kataria, D. Lis +6

PRIMA (The PRobe for-Infrared Mission for Astrophysics) is a concept for a far-infrared (IR) observatory. PRIMA features a cryogenically cooled 1.8 m diameter telescope and is desi…

astro-ph.EP20235 cited

Multiple Rings and Asymmetric Structures in the Disk of SR 21

Yi Yang, Hauyu Baobab Liu, Takayuki Muto +9

Crescent-like asymmetric dust structures discovered in protoplanetary disks indicate dust aggregations. Thus, the research on them helps us understand the planet formation process.…