activity
19972024
most citedDust formation history of galaxies: a critical role of metallicity for the dust mass growth by accreting materials in the interstellar medium

224 citations · 3.9k across the 128 of their papers we have counts for

collaborators

128 papers

astro-ph.GA2024

Radial properties of dust in galaxies: Comparison between observations and isolated galaxy simulations

S. A. van der Giessen, K. Matsumoto, M. Relano +8

We study the importance of several processes that influence the evolution of dust and its grain size distribution on spatially resolved scales in nearby galaxies. Here, we compiled…

astro-ph.GA2024

Evolution of grain size distribution in the circum-galactic medium

Hiroyuki Hirashita

In order to theoretically understand dust properties in the circum-galactic medium (CGM), we construct a dust evolution model that incorporates the evolution of grain size distribu…

astro-ph.GA2024

Dust enrichment in the circum-galactic medium

Mau Otsuki, Hiroyuki Hirashita

To understand the origin of dust in the circum-galactic medium (CGM), we develop a dust enrichment model. We describe each of the central galaxy and its CGM as a single zone, and c…

astro-ph.GA2024★ 7 cited

Observational signatures of the dust size evolution in isolated galaxy simulations

Kosei Matsumoto, Hiroyuki Hirashita, Kentaro Nagamine +9

We aim to provide observational signatures of the dust size evolution in the ISM. In particular, we explore indicators of the polycyclic aromatic hydrocarbon (PAH) mass fraction ($…

astro-ph.GA2023

Submillimetre galaxies as laboratories for dust grain coagulation

Hiroyuki Hirashita, Chian-Chou Chen

Coagulation in the dense interstellar medium (ISM) is an important process that determines the size of the largest grains. We use submillimetre galaxies (SMGs) as laboratories of g…

astro-ph.GA2023★ 7 cited

Effects of dust grain size distribution on the abundances of CO and H in galaxy evolution

Hiroyuki Hirashita

We model the effect of grain size distribution in a galaxy on the evolution of CO and H abundances. The formation and dissociation of CO and H in typical dense clouds are m…