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ALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters

dc.contributor.authorTOWNER, A.
dc.contributor.authorGINSBURG, A.
dc.contributor.authorDELL'OVA, P.
hal.structure.identifierObservatoire de Paris
dc.contributor.authorGUSDORF, A.
dc.contributor.authorBONTEMPS, S.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorCSENGERI, T.
dc.contributor.authorGALVÁN-MADRID, R.
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG]
dc.contributor.authorLOUVET, F.
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG]
dc.contributor.authorMOTTE, F.
hal.structure.identifierNational Astronomical Observatory of Japan [NAOJ]
dc.contributor.authorSANHUEZA, P.
dc.contributor.authorSTUTZ, A.
dc.contributor.authorBALLY, J.
dc.contributor.authorBAUG, T.
dc.contributor.authorCHEN, H.
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG]
dc.contributor.authorCUNNINGHAM, N.
dc.contributor.authorFERNÁNDEZ-LÓPEZ, M.
dc.contributor.authorLIU, H. -L.
dc.contributor.authorLU, X.
dc.contributor.authorNONY, T.
dc.contributor.authorVALEILLE-MANET, M.
dc.contributor.authorWU, B.
dc.contributor.authorÁLVAREZ-GUTIÉRREZ, R.
dc.contributor.authorBONFAND, M.
dc.contributor.authorDI FRANCESCO, J.
dc.contributor.authorNGUYEN-LUONG, Q.
dc.contributor.authorOLGUIN, F.
dc.contributor.authorWHITWORTH, A.
dc.date.issued2023
dc.identifier.issn0004-637X
dc.description.abstractEnWe present a catalog of 315 protostellar outflow candidates detected in SiO J=5-4 in the ALMA-IMF Large Program, observed with ~2000 au spatial resolution, 0.339 km/s velocity resolution, and 2-12 mJy/beam (0.18-0.8 K) sensitivity. We find median outflow masses, momenta, and kinetic energies of ~0.3 M$_{\odot}$, 4 M$_{\odot}$ km/s, and 10$^{45}$ erg, respectively. Median outflow lifetimes are 6,000 years, yielding median mass, momentum, and energy rates of $\dot{M}$ = 10$^{-4.4}$ M$_{\odot}$ yr$^{-1}$, $\dot{P}$ = 10$^{-3.2}$ M$_{\odot}$ km/s yr$^{-1}$, and $\dot{E}$ = 1 L$_{\odot}$. We analyze these outflow properties in the aggregate in each field. We find correlations between field-aggregated SiO outflow properties and total mass in cores (~3$-$5$σ$), and no correlations above 3$σ$ with clump mass, clump luminosity, or clump luminosity-to-mass ratio. We perform a linear regression analysis and find that the correlation between field-aggregated outflow mass and total clump mass - which has been previously described in the literature - may actually be mediated by the relationship between outflow mass and total mass in cores. We also find that the most massive SiO outflow in each field is typically responsible for only 15-30% of the total outflow mass (60% upper limit). Our data agree well with the established mechanical force-bolometric luminosity relationship in the literature, and our data extend this relationship up to L $\geq$ 10$^6$ L$_{\odot}$ and $\dot{P}$ $\geq$ 1 M$_{\odot}$ km/s yr$^{-1}$. Our lack of correlation with clump L/M is inconsistent with models of protocluster formation in which all protostars start forming at the same time.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.enAstrophysics of Galaxies (astro-ph.GA)
dc.subject.enFOS: Physical sciences
dc.title.enALMA-IMF IX: Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
dc.typeArticle de revue
dc.identifier.doi10.48550/arXiv.2310.13125
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.journalThe Astrophysical Journal
bordeaux.peerReviewedoui
hal.identifierhal-04294962
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-04294962v1
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