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20222026
most citedALMA-IMF. V. Prestellar and protostellar core populations in the W43 cloud complex

51 citations · 254 across the 18 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

astro-ph.GA2024★ 12 cited

ALMA-IMF XVI: Mass-averaged temperature of cores and protostellar luminosities in the ALMA-IMF protoclusters

F. Motte, Y. Pouteau, T. Nony +34

ALMA-IMF imaged 15 massive protoclusters down to a resolution of of 2 kau scales, identifying about 1000 star-forming cores. The mass and luminosity of these cores, which are funda…

astro-ph.GA2024★ 33 cited

ALMA-IMF XV: The core mass function in the high-mass star-formation regime

F. Louvet, P. Sanhueza, A. Stutz +38

The stellar initial mass function (IMF) is critical to our understanding of star formation and the effects of young stars on their environment. On large scales, it enables us to us…

astro-ph.GA2024

ALMA-IMF XII: Point-process mapping of 15 massive protoclusters

P. Dell'Ova, F. Motte, A. Gusdorf +29

A crucial aspect in addressing the challenge of measuring the core mass function, that is pivotal for comprehending the origin of the initial mass function, lies in constraining th…

astro-ph.GA2024★ 16 cited

ALMA-IMF XIII: NH kinematic analysis on the intermediate protocluster G353.41

R. H. Álvarez-Gutiérrez, A. M. Stutz, N. Sandoval-Garrido +23

The ALMA-IMF Large Program provides multi-tracer observations of 15 Galactic massive protoclusters at matched sensitivity and spatial resolution. We focus on the dense gas kinemati…

astro-ph.GA2024★ 25 cited

ALMA-IMF XI: The sample of hot core candidates A rich population of young high-mass proto-stars unveiled by the emission of methyl formate

M. Bonfand, T. Csengeri, S. Bontemps +28

Sites associated with high-mass star and cluster formation exhibit a so-called hot core phase, characterized by high temperatures and column densities of complex organic molecules.…

astro-ph.GA2024★ 18 cited

ALMA-IMF X -- The core population in the evolved W33-Main (G012.80) protocluster

M. Armante, A. Gusdorf, F. Louvet +21

We aimed to measure the CMF in the evolved W33-Main star-forming protocluster to compare it with CMF recently obtained in other Galactic star-forming regions, including the ones in…