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Authordc.contributor.authorHiguchi, Aya 
Authordc.contributor.authorSaigo, Kazuya 
Authordc.contributor.authorChibueze, James O. 
Authordc.contributor.authorSanhueza, Patricio 
Authordc.contributor.authorTakakuwa, Shigehisa 
Authordc.contributor.authorGaray Brignardello, Guido 
Admission datedc.date.accessioned2015-08-13T14:08:25Z
Available datedc.date.available2015-08-13T14:08:25Z
Publication datedc.date.issued2015
Cita de ítemdc.identifier.citationThe Astrophysical Journal Letters, 798:L33 (6pp), 2015 January 10en_US
Identifierdc.identifier.issn2041-8205
Identifierdc.identifier.otherDOI: 10.1088/2041-8205/798/2/L33
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/132675
General notedc.descriptionArtículo de publicación ISIen_US
Abstractdc.description.abstractWe present the results of continuum and 12CO(3–2) and CH3OH(7–6) line observations of IRAS 16547−4247 made with the Atacama Large Millimeter/submillimeter Array (ALMA) at an angular resolution of ∼0. 5. The 12CO(3–2) emission shows two high-velocity outflows whose driving sources are located within the dust continuum peak. The alignment of these outflows does not coincide with that of the wide-angle, large-scale, bipolar outflow detected with the Atacama Pathfinder Experiment in previous studies. The CH3OH(7–6) line emission traces an hourglass structure associated with the cavity walls created by the outflow lobes. Taking into account our results together with the position of the H2O and class I CH3OH maser clusters, we discuss two possible scenarios that can explain the hourglass structure observed in IRAS 16547−4247: (1) precession of a biconical jet, (2) multiple, or at least two, driving sources powering intersecting outflows. Combining the available evidence, namely, the presence of two cross-aligned bipolar outflows and two different H2O maser groups, we suggest that IRAS 16547−4247 represents an early formation phase of a protocluster.en_US
Patrocinadordc.description.sponsorshipCONICYT project PFB-06en_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherAmerican Astronomical Societyen_US
Type of licensedc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectISM: individual objects (IRAS 16547−4247)en_US
Keywordsdc.subjectISM: jets and outflowsen_US
Keywordsdc.subjectISM: kinematics and dynamicsen_US
Keywordsdc.subjectISM: moleculesen_US
Keywordsdc.subjectStars: formationen_US
Keywordsdc.subjectStars: massiveen_US
Títulodc.titleIRAS 16547−4247: A New Candidate of a Protocluster Unveiled with ALMAen_US
Document typedc.typeArtículo de revistaen_US


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Atribución-NoComercial-SinDerivadas 3.0 Chile
Except where otherwise noted, this item's license is described as Atribución-NoComercial-SinDerivadas 3.0 Chile