activity
20142025
most citedReprocessing of Ices in Turbulent Protoplanetary Disks: Carbon and Nitrogen Chemistry

135 citations · 504 across the 30 of their papers we have counts for

collaborators

28 papers

astro-ph.EP20252 cited

Winding Motion of Spirals in a Gravitationally Unstable Protoplanetary Disk

Tomohiro C. Yoshida, Hideko Nomura, Kiyoaki Doi +5

The discovery of wide-orbit giant exoplanets has posed a challenge to our conventional understanding of planet formation by coagulation of dust grains and planetesimals, and subseq…

astro-ph.GA2025

Formation of unsaturated carbon chains through carbon chemisorption on solid CO

Masashi Tsuge, Germán Molpeceres, Ryota Ichimura +3

The interaction of carbon atoms with solid carbon monoxide (CO) is a fundamental process in astrochemistry, influencing the formation of complex organic molecules in interstellar e…

astro-ph.GA20253 cited

Extended and Compact Ortho-HD Structures Close to the Moment of Star-Formation: Evidence from ALMA-ACA Observations in Taurus

Kazuki Tokuda, Kenji Furuya, Naofumi Fukaya +8

Observing and characterizing pre- and protostellar cores in the earliest and densest stages of star formation is challenging due to their short timescales and high densities, limit…

astro-ph.GA2025

Binding energy distributions of alcohols, thiols, and their precursors on interstellar water ice surfaces

Arghyadeb Roy, Ankan Das, Milan Sil +4

Binding energy (BE) is a critical parameter in astrochemical modeling, governing the retention of species on interstellar dust grains and their subsequent chemical evolution. Howev…

astro-ph.GA2025

The detection of spatially resolved protosteller outflows and episodic jets in the outer Galaxy

Toki Ikeda, Takashi Shimonishi, Natsuko Izumi +5

We present the first detection of spatially resolved protostellar outflows and jets in the outer Galaxy. We observed five star-forming regions in the outer Galaxy (Sh 2--283, NOMF0…

astro-ph.EP2024

Dust Scattering Albedo at Millimeter-Wavelengths in the TW Hya Disk

Tomohiro C. Yoshida, Hideko Nomura, Takashi Tsukagoshi +3

Planetary bodies are formed by coagulation of solid dust grains in protoplanetary disks. Therefore, it is crucial to constrain the physical and chemical properties of the dust grai…