output
19942026
most citedMass Estimates of a Giant Planet in a Protoplanetary Disk from the Gap Structures

210 citations

Showing astro-ph.GAShow all

12 papers · 1 filter

astro-ph.GA2025★ 2 cited

The First Star-by-star -body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model

Keiya Hirashima, Michiko S. Fujii, Takayuki R. Saitoh +9

A major goal of computational astrophysics is to simulate the Milky Way Galaxy with sufficient resolution down to individual stars. However, the scaling fails due to some small-sca…

astro-ph.GA2024★ 5 cited

Hydrogenation of acetaldehyde on interstellar ice analogs reveals limited destruction

Germán Molpeceres, Thanh Nguyen, Yasuhiro Oba +1

We sought to determine which are the main hydrogenation paths of acetaldehyde (CH3CHO). As a partially unsaturated molecule, CH3CHO can have links with more hydrogenated species, l…

astro-ph.GA2024★ 28 cited

Violent starbursts and quiescence induced by FUV radiation feedback in metal-poor galaxies at high-redshift

Kazuyuki Sugimura, Massimo Ricotti, Jongwon Park +2

JWST observations of galaxies at suggest that they are more luminous and clumpier than predicted by most models, prompting several proposals on the physics of star for…

astro-ph.GA2023★ 24 cited

Modelling Deuterated Isotopologues of Methanol toward the Pre-Stellar Core L1544

W. Riedel, O. Sipilä, E. Redaelli +4

Aims. We aim to improve a previous model for the prediction of column densities and deuterium fractions of non- and singly deuterated methanol. Thereby, we try to identify crucial…

astro-ph.GA2023★ 8 cited

Determination of the branching ratio of CHOH + OH reaction on water ice surface at 10 K

Atsuki Ishibashi, Hiroshi Hidaka, W. M. C. Sameera +2

The CHO and CHOH radicals can be important precursors of complex organic molecules (COMs) in interstellar dust. The COMs presumably originating from these radicals were abu…

astro-ph.GA2022★ 21 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.GA2022★ 6 cited

Penetration of Non-energetic Hydrogen Atoms into Amorphous Solid Water and their Reaction with Embedded Benzene and Naphthalene

Masashi Tsuge, Akira Kouchi, Naoki Watanabe

Chemical processes on the surface of icy grains play an important role in the chemical evolution in molecular clouds. In particular, reactions involving non-energetic hydrogen atom…

astro-ph.GA2021★ 10 cited

Measurements of Ortho-to-para Nuclear Spin Conversion of H2 on Low-temperature Carbonaceous Grain Analogues: Diamond-like Carbon and Graphite

Masashi Tsuge, Akira Kouchi, Naoki Watanabe

Hydrogen molecules have two nuclear spin isomers: ortho-H2 and para-H2. The ortho-to-para ratio (OPR) is known to affect chemical evolution as well as gas dynamics in space. Theref…

astro-ph.GA2021★ 36 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.GA2021★ 13 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.GA2018★ 51 cited

Thermal desorption of formamide and methylamine from graphite and amorphous water ice surfaces

Henda Chaabouni, Stephan Diana, Thanh Nguyen +1

Formamide (NH2CHO) and methylamine (CH3NH2) are known to be the most abundant amine-containing molecules in many astrophysical environments. The presence of these molecules in the…

astro-ph.GA2012★ 109 cited

Water Formation through a Quantum Tunneling Surface Reaction, OH + H2, at 10 K

Y. Oba, N. Watanabe, T. Hama +3

The present study experimentally demonstrated that solid H2O is formed through the surface reaction OH + H2 at 10 K. This is the first experimental evidence of solid H2O formation…