activity
20042023
most citedCharacterizing interstellar filaments with Herschel in IC5146

792 citations · 6.8k across the 87 of their papers we have counts for

collaborators

85 papers

astro-ph.GA2023★ 19 cited

Unveiling the formation of the massive DR21 ridge

L. Bonne, S. Bontemps, N. Schneider +10

We present new CO(1-0), CO(1-0), HCO(1-0) and HCO(1-0) maps from the IRAM 30m telescope, and a spectrally-resolved [CII] 158 m map observed with…

astro-ph.GA2023★ 32 cited

Ionized carbon as a tracer of the assembly of interstellar clouds

Nicola Schneider, Lars Bonne, Sylvain Bontemps +9

Molecular hydrogen clouds are a key component of the interstellar medium because they are the birthplaces for stars. They are embedded in atomic gas that pervades the interstellar…

astro-ph.GA2022★ 46 cited

ALMA-IMF VI -- Investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&MM3 mini-starburst

Y. Pouteau, F. Motte, T. Nony +35

Among the most central open questions regarding the initial mass function (IMF) of stars is the impact of environment on the shape of the core mass function (CMF) and thus potentia…

astro-ph.GA2022★ 16 cited

CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A

Hideaki Takemura, Fumitaka Nakamura, Héctor G. Arce +15

The mass distribution of dense cores is a potential key to understand the process of star formation. Applying dendrogram analysis to the CARMA-NRO Orion CO (=1--0) data,…

astro-ph.GA2022★ 8 cited

A Herschel study of G214.5-1.8: a young, cold and quiescent giant molecular filament on the shell of a HI superbubble

S. D. Clarke, A. Sanchez-Monge, G. M. Williams +3

We present an analysis of the outer Galaxy giant molecular filament (GMF) G214.5-1.8 (G214.5) using Herschel data. We find that G214.5 has a mass of 16,000 M, yet…

astro-ph.GA2022★ 8 cited

SOFIA FEEDBACK survey: PDR diagnostics of stellar feedback in different regions of RCW 49

M. Tiwari, M. Wolfire, M. W. Pound +13

We quantified the effects of stellar feedback in RCW 49 by determining the physical conditions in different regions using the [CII] 158 m and [OI] 63 m observations from SOFI…