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dc.contributor.authorDÍAZ-GONZÁLEZ, Daniel
dc.contributor.authorGALVÁN-MADRID, Roberto
dc.contributor.authorGINSBURG, Adam
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG]
dc.contributor.authorMOTTE, Frédérique
hal.structure.identifierAstrophysique
dc.contributor.authorDELL'OVA, Pierre
dc.contributor.authorKURTZ, Stan
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG]
dc.contributor.authorCUNNINGHAM, Nichol
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorSTUTZ, Amelia
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG]
dc.contributor.authorLOUVET, Fabien
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
dc.contributor.authorCSENGERI, Timea
hal.structure.identifierConsejo Superior de Investigaciones Cientificas [España] = Spanish National Research Council [Spain] [CSIC]
dc.contributor.authorFERNÁNDEZ-LÓPEZ, Manuel
hal.structure.identifierNational Astronomical Observatory of Japan [NAOJ]
hal.structure.identifierGraduate University for Advanced Studies [Hayama] [SOKENDAI]
dc.contributor.authorSANHUEZA, Patricio
dc.contributor.authorNONY, Thomas
dc.contributor.authorRIVERA-SOTO, Rudy
dc.contributor.authorÁLVAREZ-GUTIÉRREZ, Rodrigo
dc.contributor.authorARMANTE, Melanie
dc.contributor.authorBONFAND, Melisse
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
dc.contributor.authorBONTEMPS, Sylvain
hal.structure.identifierAstrophysique
hal.structure.identifierLERMA Cergy [LERMA]
dc.contributor.authorGUSDORF, Antoine
hal.structure.identifierYunnan University
dc.contributor.authorLIU, Hong-Li
dc.date.issued2023
dc.identifier.issn0067-0049
dc.description.abstractEnWe present the combination of ALMA-IMF and single-dish continuum images from the Mustang-2 Galactic Plane Survey (MGPS90) at 3 millimeters and the Bolocam Galactic Plane Survey (BGPS) at 1 millimeter. Six and ten out of the fiffteen ALMA-IMF fields are combined with MGPS90 and BGPS, respectively. The combination is made via the feathering technique. We used the dendrogram algorithm throughout the combined images, and performed further analysis in the six fields with combination in both bands (G012.80, W43-MM1, W43-MM2, W43-MM3, W51-E, W51-IRS2). In these fields, we calculated spectral index maps and used them to separate regions dominated by dust or free-free emission, and then performed further structural analysis. We report the basic physical parameters of the dust-dominated (column densities, masses) and ionized (emission measures, hydrogen ionization photon rates) structures. We also searched for multi-scale relations in the dust-dominated structures across the analyzed fields, finding that the fraction of mass in dendrogram leaves (which we label as "Leaf Mass Eficiency", LME) as a function of molecular gas column density follows a similar trend: a rapid, exponential-like growth, with maximum values approaching 100% in most cases. The observed behaviour of the LME with gas column is tentatively interpreted as an indicator of large star formation activity within the ALMA-IMF protoclusters. W51-E and G012.80 stand out as cases with comparatively large and reduced potential for further star formation, respectively.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enAstrophysics of Galaxies (astro-ph.GA)
dc.title.enALMA-IMF VIII -- Combination of Interferometric Continuum Images with Single-Dish Surveys and Structural Analysis of Six Protoclusters
dc.typeArticle de revue
dc.identifier.doi10.48550/arXiv.2310.13872
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.journalThe Astrophysical Journal Supplement
bordeaux.peerReviewedoui
hal.identifierhal-04290564
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-04290564v1
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