activity
20182022
most citedALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first results

95 citations · 284 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2022★ 19 cited

ALMA-IMF IV -- A comparative study of the main hot cores in W43-MM1: detection, temperature and molecular composition

N. Brouillet, D. Despois, J. Molet +21

W43-MM1 is a young region, very rich in terms of high-mass star formation. We aim to systematically identify the massive cores which contain a hot core and compare their molecular…

astro-ph.GA2021★ 95 cited

ALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first results

F. Motte, S. Bontemps, T. Csengeri +61

The ALMA-IMF Large Program imaged a total noncontiguous area of 53pc2, covering 15 extreme, nearby protoclusters of the Milky Way. They were selected to span relevant early protocl…

astro-ph.GA2021★ 39 cited

ALMA-IMF II -- investigating the origin of stellar masses: Continuum Images and Data Processing

A. Ginsburg, T. Csengeri, R. Galván-Madrid +49

We present the first data release of the ALMA-IMF Large Program, which covers the 12m-array continuum calibration and imaging. The ALMA-IMF Large Program is a survey of fifteen den…

astro-ph.GA2020★ 52 cited

Episodic accretion constrained by a rich cluster of outflows

T. Nony, F. Motte, F. Louvet +8

The accretion history of protostars remains widely mysterious even though it represents one of the best ways to understand the protostellar collapse that leads to the formation of…

astro-ph.GA2019★ 32 cited

Molecular analysis of a high-mass prestellar core candidate in W43-MM1

J. Molet, N. Brouillet, T. Nony +6

High-mass analogues of low-mass prestellar cores are searched for to constrain the models of high-mass star formation. Several high-mass cores, at various evolutionary stages, have…

astro-ph.GA2018★ 47 cited

Detection of a high-mass prestellar core candidate in W43-MM1

T. Nony, F. Louvet, F. Motte +11

Aims. To constrain the physical processes that lead to the birth of high-mass stars it is mandatory to study the very first stages of their formation. We search for high-mass analo…