activity
20162022
most citedALMA survey of Class II protoplanetary disks in Corona Australis: a young region with low disk masses

93 citations · 434 across the 25 of their papers we have counts for

collaborators

43 papers

astro-ph.SR202239 cited

A likely flyby of binary protostar Z CMa caught in action

Ruobing Dong, Hauyu Baobab Liu, Nicolas Cuello +16

Close encounters between young stellar objects in star forming clusters are expected to dramatically perturb circumstellar disks. Such events are witnessed in numerical simulations…

astro-ph.EP202218 cited

Determining dispersal mechanisms of protoplanetary disks using accretion and wind mass loss rates

Yasuhiro Hasegawa, Thomas J. Haworth, Keri Hoadley +6

Understanding the origin of accretion and dispersal of protoplanetary disks is fundamental for investigating planet formation. Recent numerical simulations show that launching wind…

astro-ph.EP202119 cited

Keck/OSIRIS Pa high-contrast imaging and updated constraints on PDS~70b

Taichi Uyama, Chen Xie, Yuhiko Aoyama +11

We present a high-contrast imaging search for Pa line emission from protoplanets in the PDS~70 system with Keck/OSIRIS integral field spectroscopy. We applied the high-resolutio…

astro-ph.EP20212 cited

The architecture of multi-planet systems as a tracer of their formation mechanisms

Udit Arora, Yasuhiro Hasegawa

Exoplanets observed by the {\it Kepler} telescope exhibit a bi-modal, radius distribution, which is known as the radius gap. We explore an origin of the radius gap, focusing on mul…

astro-ph.EP2021

Formation of rims around chondrules via porous aggregate accretion

Yuji Matsumoto, Yasuhiro Hasegawa, Nozomi Matsuda +1

Chondrules are often surrounded by fine-grained rims or igneous rims. The properties of these rims reflect their formation histories. While the formation of fine-grained rims is mo…

astro-ph.EP202132 cited

ALMA Observations of the Asymmetric Dust Disk around DM Tau

Jun Hashimoto, Takayuki Muto, Ruobing Dong +5

We report an analysis of the dust disk around DM~Tau, newly observed with the Atacama Large Millimeter/submillimeter Array (ALMA) at 1.3 mm. The ALMA observations with high sensiti…