The ALPINE-ALMA [CII] Survey: A Triple Merger at z ~ 4.56

dc.contributor.authorIbar, Eduardo
dc.date.accessioned2021-07-22T17:11:24Z
dc.date.available2021-07-22T17:11:24Z
dc.date.issued2020
dc.description.abstractWe report the detection of [C II] λ158 μm emission from a system of three closely separated sources in the Cosmic Evolution Survey (COSMOS) field at z ∼ 4.56 , as part of the Atacama Large Millimeter/submillimeter Array (ALMA) Large Program to INvestigate C II at Early times (ALPINE). The two most luminous sources are closely associated, both spatially (1.6 arcsec ∼ 11 kpc) and in velocity (∼100 km s−1), while the third source is slightly more distant (2.8 arcsec ∼ 18 kpc, ∼300 km s−1). The second most luminous source features a slight velocity gradient, while no significant velocity gradient is seen in the other two sources. Using the observed [C II] luminosities, we derive a total log10(SFR[CII][M⊙yr−1])=2.8±0.2⁠, which may be split into contributions of 59, 31, and 10 per cent from the central, east, and west sources, respectively. Comparison of these [C II] detections to recent zoom-in cosmological simulations suggests an ongoing major merger. We are thus witnessing a system in a major phase of mass build-up by merging, including an ongoing major merger and an upcoming minor merger, which is expected to end up in a single massive galaxy by z ∼ 2.5.en_ES
dc.identifier.doihttps://doi.org/10.1093/mnrasl/slz154
dc.identifier.urihttp://repositoriobibliotecas.uv.cl/handle/uvscl/2148
dc.language.isoenen_ES
dc.publisherRoyal Astronomical Societyen_ES
dc.sourceMonthly Notices of the Royal Astronomical Society: Lettersen_ES
dc.subjectGALAXIES: EVOLUTIONen_ES
dc.subjectGALAXIES: HIGH-REDSHIFTen_ES
dc.subjectGALAXIES: INTERACTIONSen_ES
dc.subjectGALAXIES: KINEMATICS AND DYNAMICSen_ES
dc.titleThe ALPINE-ALMA [CII] Survey: A Triple Merger at z ~ 4.56en_ES
dc.typeArticuloen_ES
uv.catalogadorRCR DIBRAen_ES
uv.notageneralVarios autoresen_ES

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