activity
20192022
most citedTransmission Electron Microscopy Study of the Morphology of Ices Composed of H2O, CO2, and CO on Refractory Grains

36 citations · 116 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202221 cited

Direct Determination of the Activation Energy for Diffusion of OH Radicals on Water Ice

A. Miyazaki, M. Tsuge, H. Hidaka +2

Using a combination of photostimulated desorption and resonance-enhanced multiphoton ionization methods, the behaviors of OH radicals on the surface of interstellar ice analog was…

astro-ph.GA202136 cited

Transmission Electron Microscopy Study of the Morphology of Ices Composed of H2O, CO2, and CO on Refractory Grains

Akira Kouchi, Masashi Tsuge, Tetsuya Hama +15

It has been implicitly assumed that ices on grains in molecular clouds and proto planetary disks are formed by homogeneous layers regardless of their composition or crystallinity.…

astro-ph.GA202130 cited

Behavior of Hydroxyl Radicals on Water Ice at Low Temperatures

Masashi Tsuge, Naoki Watanabe

Because chemical reactions on/in cosmic ice dust grains covered by amorphous solid water (ASW) play important roles in generating a variety of molecules, many experimental and theo…

astro-ph.GA202113 cited

Rapid ortho-to-para nuclear spin conversion of H2 on a silicate dust surface

Masashi Tsuge, Toshinobu Namiyoshi, Kenji Furuya +3

The H2 molecule has two nuclear spin isomers, the so-called ortho and para isomers. Nuclear spin conversion (NSC) between these states is forbidden in the gas phase. The energy dif…

astro-ph.GA2020

Diffusive hydrogenation reactions of CO embedded in amorphous solid water at elevated temperatures ~70 K

Masashi Tsuge, Hiroshi Hidaka, Akira Kouchi +1

The surface processes on interstellar dust grains have an important role in the chemical evolution in molecular clouds. Hydrogenation reactions on ice surfaces have been extensivel…

astro-ph.GA201916 cited

Interactions of Atomic and Molecular Hydrogen with a Diamond-like Carbon Surface: H2 Formation and Desorption

Masashi Tsuge, Tetsuya Hama, Yuki Kimura +2

The interactions of atomic and molecular hydrogen with bare interstellar dust grain surfaces are important for understanding H2 formation at relatively high temperatures (>20 K). W…