MORPHOLOGY AND MOLECULAR GAS FRACTIONS OF LOCAL LUMINOUS INFRARED GALAXIES AS A FUNCTION OF INFRARED LUMINOSITY AND MERGER STAGE
dc.contributor.author | Larson, K. L. | |
dc.contributor.author | Sanders, D. B. | |
dc.contributor.author | Barnes, J. E. | |
dc.contributor.author | Ishida, C. M. | |
dc.contributor.author | Evans, A. S. | |
dc.contributor.author | Mazzarella, J. M. | |
dc.contributor.author | Kim, D. C. | |
dc.contributor.author | Privon, G. C. | |
dc.contributor.author | Mirabel, I. F. | |
dc.contributor.author | Flewelling, H. A. | |
dc.date.accessioned | 2024-01-10T12:40:38Z | |
dc.date.available | 2024-01-10T12:40:38Z | |
dc.date.issued | 2016 | |
dc.description.abstract | We present a new, detailed analysis of the morphologies and molecular gas fractions (MGFs) for a complete sample of 65 local luminous infrared galaxies from Great Observatories All-Sky Luminous Infrared Galaxies (LIRG) Survey using high resolution I-band images from The Hubble Space Telescope, the University of Hawaii 2.2 m Telescope and the Pan-STARRS1 Survey. Our classification scheme includes single undisturbed galaxies, minor mergers, and major mergers, with the latter divided into five distinct stages from pre-first pericenter passage to final nuclear coalescence. We find that major mergers of molecular gas-rich spirals clearly play a major role for all sources with L-IR > 10(11.5)L(circle dot); however, below this luminosity threshold, minor mergers and secular processes dominate. Additionally, galaxies do not reach L-IR > 10(12.0)L(circle dot) until late in the merger process when both disks are near final coalescence. The mean MGF (MGF = M-H2(M*+ M-H2)) for non-interacting and early-stage major merger LIRGs is 18 +/- 2%, which increases to 33 +/- 3%, for intermediate stage major merger LIRGs, consistent with the hypothesis that, during the early-mid stages of major mergers, most of the initial large reservoir of atomic gas (HI) at large galactocentric radii is swept inward where it is converted into molecular gas (H-2). | |
dc.description.funder | National Science Foundation | |
dc.description.funder | Distinguished Visitor Program at the Research School for Astronomy and Astrophysics, Australian National University | |
dc.description.funder | NASA grant | |
dc.description.funder | Thirty Meter Telescope International Observatory | |
dc.description.funder | UC Chancellor's Postdoctoral Fellowship Program | |
dc.description.funder | NSF grant | |
dc.description.funder | Taiwan, R.O.C. Ministry of Science and Technology grant | |
dc.description.funder | FONDECYT Postdoctoral Fellowship | |
dc.description.funder | UH TAC | |
dc.description.funder | National Aeronautics and Space Administration through Planetary Science Division of the NASA Science Mission Directorate | |
dc.fechaingreso.objetodigital | 2024-05-30 | |
dc.format.extent | 16 páginas | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.3847/0004-637X/825/2/128 | |
dc.identifier.eissn | 1538-4357 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.uri | https://doi.org/10.3847/0004-637X/825/2/128 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/77331 | |
dc.identifier.wosid | WOS:000381940800046 | |
dc.information.autoruc | Física;Privon G;S/I;1031484 | |
dc.issue.numero | 2 | |
dc.language.iso | en | |
dc.nota.acceso | Contenido parcial | |
dc.publisher | IOP PUBLISHING LTD | |
dc.revista | ASTROPHYSICAL JOURNAL | |
dc.rights | acceso restringido | |
dc.subject | galaxies: evolution | |
dc.subject | galaxies: interactions | |
dc.subject | infrared: galaxies | |
dc.subject | MERGING GALAXIES | |
dc.subject | ULTRALUMINOUS GALAXIES | |
dc.subject | INTERSTELLAR-MEDIUM | |
dc.subject | ANTENNAE GALAXIES | |
dc.subject | CONVERSION FACTOR | |
dc.subject | MAJOR MERGERS | |
dc.subject | DISK GALAXIES | |
dc.subject | HERSCHEL-PACS | |
dc.subject | GREAT DEBATE | |
dc.subject | GOALS SAMPLE | |
dc.title | MORPHOLOGY AND MOLECULAR GAS FRACTIONS OF LOCAL LUMINOUS INFRARED GALAXIES AS A FUNCTION OF INFRARED LUMINOSITY AND MERGER STAGE | |
dc.type | artículo | |
dc.volumen | 825 | |
sipa.codpersvinculados | 1031484 | |
sipa.index | WOS | |
sipa.index | Scopus | |
sipa.trazabilidad | Carga SIPA;09-01-2024 |
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