activity
20042026
most citedThe fate of the interstellar medium in early-type galaxies. I. First direct measurement of the timescale of dust removal

33 citations · 51 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026★ 1 cited

Ion-Neutral Drift Velocity as a Diagnostic of Dust Growth and Magnetic Field in Star-Forming Environments

Haruka Fukihara, Yusuke Tsukamoto, Hiroyuki Hirashita +2

Recent observations have revealed that the ion-neutral drift velocity in star-forming molecular clouds and dense cores is on the order of 100 m s^-1. Theoretical studies have shown…

astro-ph.GA2024★ 2 cited

CO-to-H conversion factor and grain size distribution through the analysis of - relation

I-Da Chiang, Hiroyuki Hirashita, Jeremy Chastenet +5

The CO-to-H conversion factor () is expected to vary with dust abundance and grain size distribution through the efficiency of shielding gas from CO-dissociation…

astro-ph.GA2024★ 15 cited

JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium

Jérémy Chastenet, Ilse De Looze, Monica Relaño +37

We present new JWST observations of the nearby, prototypical edge-on, spiral galaxy NGC 891. The northern half of the disk was observed with NIRCam in its F150W and F277W filters.…

astro-ph.GA2024

Accurate Simultaneous Constraints on the Dust Mass, Temperature and Emissivity Index of a Galaxy at Redshift 7.31

Hiddo Algera, Hanae Inami, Ilse De Looze +21

We present new multi-frequency ALMA continuum observations of the massive [], UV-luminous [] $z=7.31…

astro-ph.GA2019★ 33 cited

The fate of the interstellar medium in early-type galaxies. I. First direct measurement of the timescale of dust removal

Michał J. Michałowski, J. Hjorth, C. Gall +12

An important aspect of quenching star formation is the removal of the cold interstellar medium (ISM; non-ionised gas and dust) from a galaxy. In addition, dust grains can be destro…

astro-ph.GA2016

The infrared-dark dust content of high redshift galaxies

A. Ferrara, H. Hirashita, M. Ouchi +1

We present a theoretical model aimed at explaining the IRX- relation for high redshift (z >5) galaxies. Recent observations (Capak+2015; Bouwens+2016) have shown that early Lyma…