activity
20142023
most citedProbing accretion of ambient cloud material into the Taurus B211/B213 filament

76 citations · 267 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023★ 23 cited

Witnessing the fragmentation of a filament into prestellar cores in Orion B/NGC 2024

Y. Shimajiri, Ph. André, N. Peretto +3

Recent Herschel observations of nearby clouds have shown that filamentary structures are ubiquitous and that most prestellar cores form in filaments. Probing the density () and…

astro-ph.GA2021★ 45 cited

The width of Herschel filaments varies with distance

G. V. Panopoulou, S. E. Clark, A. Hacar +5

Context: Filamentary structures in nearby molecular clouds have been found to exhibit a characteristic width of 0.1 pc, as observed in dust emission. Understanding the origin of th…

astro-ph.GA2019★ 53 cited

Probing fragmentation and velocity sub-structure in the massive NGC 6334 filament with ALMA

Y. Shimajiri, Ph. Andre, E. Ntormousi +3

Herschel surveys of Galactic clouds support a paradigm for low-mass star formation in which dense filaments play a crucial role. The detailed fragmentation properties of star-formi…

astro-ph.GA2018★ 76 cited

Probing accretion of ambient cloud material into the Taurus B211/B213 filament

Y. Shimajiri, Ph. Andre, P. Palmeirim +5

Herschel observations have emphasized the role of molecular filaments in star formation. However, the origin and evolution of these filaments are not yet well understood, partly be…

astro-ph.SR2014★ 70 cited

Age, size, and position of H ii regions in the Galaxy. Expansion of ionized gas in turbulent molecular clouds

P. Tremblin, L. D. Anderson, P. Didelon +8

This work aims at improving the current understanding of the interaction between H ii regions and turbulent molecular clouds. We propose a new method to determine the age of a larg…