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dc.contributor.author
Pouteau, Y.
dc.contributor.author
Motte, F.
dc.contributor.author
Nony, T.
dc.contributor.author
González, M.
dc.contributor.author
Joncour, I.
dc.contributor.author
Robitaille, J.-F.
dc.contributor.author
Busquet, G.
dc.contributor.author
Galván Madrid, R.
dc.contributor.author
Gusdorf, A.
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Hennebelle, P.
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Ginsburg, A.
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Csengeri, T.
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Sanhueza, P.
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Dell'Ova, P.
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Stutz, A. M.
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Towner, A. P. M.
dc.contributor.author
Cunningham, N.
dc.contributor.author
Louvet, F.
dc.contributor.author
Men?shchikov, A.
dc.contributor.author
Fernandez Lopez, Manuel
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dc.contributor.author
Schneider, N.
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Armante, M.
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Bally, J.
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Baug, T.
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Bonfand, M.
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Bontemps, S.
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Bronfman, L.
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Brouillet, N.
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Díaz-González, D.
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Herpin, F.
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Lefloch, B.
dc.contributor.author
Liu, H.-L.
dc.contributor.author
Lu, X.
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Nakamura, F.
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Luong, Q. Nguyen
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Olguin, F.
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Tatematsu, K.
dc.contributor.author
Valeille Manet, M.
dc.date.available
2023-12-01T16:08:46Z
dc.date.issued
2023-06
dc.identifier.citation
Pouteau, Y.; Motte, F.; Nony, T.; González, M.; Joncour, I.; et al.; ALMA-IMF. VI : investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&MM3 mini-starburst; EDP Sciences; Astronomy and Astrophysics; 674; 6-2023
dc.identifier.issn
0004-6361
dc.identifier.uri
http://hdl.handle.net/11336/219053
dc.description.abstract
Context. 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 potentially on the IMF.Aims: The ALMA-IMF Large Program aims to investigate the variations in the core distributions (CMF and mass segregation) with cloud characteristics, such as the density and kinematic of the gas, as diagnostic observables of the formation process and evolution of clouds. The present study focuses on the W43-MM2&MM3 mini-starburst, whose CMF has recently been found to be top-heavy with respect to the Salpeter slope of the canonical IMF.Methods: W43-MM2&MM3 is a useful test case for environmental studies because it harbors a rich cluster that contains a statistically significant number of cores (specifically, 205 cores), which was previously characterized in Paper III. We applied a multi-scale decomposition technique to the ALMA 1.3 mm and 3 mm continuum images of W43-MM2&MM3 to define six subregions, each 0.5-1 pc in size. For each subregion we characterized the probability distribution function of the high column density gas, η-PDF, using the 1.3 mm images. Using the core catalog, we investigate correlations between the CMF and cloud and core properties, such as the η-PDF and the core mass segregation.Results: We classify the W43-MM2&MM3 subregions into different stages of evolution, from quiescent to burst to post-burst, based on the surface number density of cores, number of outflows, and ultra-compact HII presence. The high-mass end (>1 M⊙) of the subregion CMFs varies from close to the Salpeter slope (quiescent) to top-heavy (burst and post-burst). Moreover, the second tail of the η-PDF varies from steep (quiescent) to flat (burst and post-burst), as observed for high-mass star-forming clouds. We find that subregions with flat second η-PDF tails display top-heavy CMFs.Conclusions: In dynamical environments such as W43-MM2&MM3, the high-mass end of the CMF appears to be rooted in the cloud structure, which is at high column density and surrounds cores. This connection stems from the fact that cores and their immediate surroundings are both determined and shaped by the cloud formation process, the current evolutionary state of the cloud, and, more broadly, the star formation history. The CMF may evolve from Salpeter to top-heavy throughout the star formation process from the quiescent to the burst phase. This scenario raises the question of if the CMF might revert again to Salpeter as the cloud approaches the end of its star formation stage, a hypothesis that remains to be tested.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
EDP Sciences
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dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
stars: formation
dc.subject
stars: massive
dc.subject
ISM: clouds
dc.subject
submillimeter: ISM
dc.subject.classification
Astronomía
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dc.subject.classification
Ciencias Físicas
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dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
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dc.title
ALMA-IMF. VI : investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&MM3 mini-starburst
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2023-11-13T15:50:59Z
dc.journal.volume
674
dc.journal.pais
Francia
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dc.description.fil
Fil: Pouteau, Y.. Universite Grenoble Alpes; Francia
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Fil: Motte, F.. Universite Grenoble Alpes; Francia
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Fil: Nony, T.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
dc.description.fil
Fil: González, M.. Universite Grenoble Alpes; Francia
dc.description.fil
Fil: Joncour, I.. Universite Grenoble Alpes; Francia
dc.description.fil
Fil: Robitaille, J.-F.. Universite Grenoble Alpes; Francia
dc.description.fil
Fil: Busquet, G.. Universidad de Barcelona; España
dc.description.fil
Fil: Galván Madrid, R.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
dc.description.fil
Fil: Gusdorf, A.. Universite Paris-Saclay; Francia
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Fil: Hennebelle, P.. Universite Paris-Saclay; Francia
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Fil: Ginsburg, A.. University of Virginia; Estados Unidos
dc.description.fil
Fil: Csengeri, T.. Universite Paris-Saclay; Francia
dc.description.fil
Fil: Sanhueza, P.. National Astronomical Observatory of Japan; Japón
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Fil: Dell'Ova, P.. Universite Paris-Saclay; Francia
dc.description.fil
Fil: Stutz, A. M.. Universidad de Concepción; Chile
dc.description.fil
Fil: Towner, A. P. M.. University of Virginia; Estados Unidos
dc.description.fil
Fil: Cunningham, N.. Universite Grenoble Alpes; Francia
dc.description.fil
Fil: Louvet, F.. Universite Grenoble Alpes; Francia
dc.description.fil
Fil: Men?shchikov, A.. Universite Paris-Saclay; Francia
dc.description.fil
Fil: Fernandez Lopez, Manuel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
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Fil: Schneider, N.. Max Planck Institute For Extraterrestrial Physics; Alemania
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Fil: Armante, M.. Universite Paris-Saclay; Francia
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Fil: Bally, J.. University of Maryland; Estados Unidos
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Fil: Baug, T.. Academia Sinica; China
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Fil: Bonfand, M.. Universite de Bordeaux; Francia
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Fil: Bontemps, S.. Universite de Bordeaux; Francia
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Fil: Bronfman, L.. Universidad de Chile; Chile
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Fil: Brouillet, N.. Universite de Bordeaux; Francia
dc.description.fil
Fil: Díaz-González, D.. Universidad Autónoma de méxico. Instituto de Radioastronomía y Astrofísica; México
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Fil: Herpin, F.. Universite de Bordeaux; Francia
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Fil: Lefloch, B.. Universite de Bordeaux; Francia
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Fil: Liu, H.-L.. Academia Sinica; China
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Fil: Lu, X.. Academia Sinica; China
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Fil: Nakamura, F.. National Astronomical Observatory of Japan; Japón
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Fil: Luong, Q. Nguyen. National Tsing Hua University; China
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Fil: Olguin, F.. National Tsing Hua University; China
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Fil: Tatematsu, K.. National Astronomical Observatory Of Japan; Japón
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Fil: Valeille Manet, M.. Universite de Bordeaux; Francia
dc.journal.title
Astronomy and Astrophysics
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dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/10.1051/0004-6361/202244776
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1051/0004-6361/202244776
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