Extreme CO Isotopic Abundances in the ULIRG IRAS 13120-5453: An Extremely Young Starburst or Top-heavy Initial Mass Function
dc.contributor.author | Sliwa, Kazimierz | |
dc.contributor.author | Wilson, Christine D. | |
dc.contributor.author | Aalto, Susanne | |
dc.contributor.author | Privon, George C. | |
dc.date.accessioned | 2024-01-10T12:05:26Z | |
dc.date.available | 2024-01-10T12:05:26Z | |
dc.date.issued | 2017 | |
dc.description.abstract | We present ALMA (CO)-C-12 (J = 1-0, 3-2 and 6-5), (CO)-C-13(J = 1-0), and (CO)-O-18 (J = 1-0) observations of the local ultraluminous infrared galaxy (ULIRG) IRAS. 13120-5453. The morphologies of the three isotopic species differ, as (CO)-C-13 shows a hole in emission toward the center. We measure integrated brightness temperature line ratios of (CO)-C-12/(CO)-C-13 >= 60 (exceeding 200) and (CO)-C-13/(CO)-O-18 <= 1 in the central region. Assuming optical thin emission, (CO)-O-18 is more abundant than (CO)-C-13 in several regions. The abundances within the central 500 pc are consistent with the enrichment of the interstellar medium via a young starburst(<7 Myr), a top-heavy initial mass function, or a combination of both. | |
dc.description.funder | FONDECYT Postdoctoral Fellowship | |
dc.fechaingreso.objetodigital | 2024-05-30 | |
dc.format.extent | 6 páginas | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.3847/2041-8213/aa6ea4 | |
dc.identifier.eissn | 2041-8213 | |
dc.identifier.issn | 2041-8205 | |
dc.identifier.uri | https://doi.org/10.3847/2041-8213/aa6ea4 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/76008 | |
dc.identifier.wosid | WOS:000400976500001 | |
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 LETTERS | |
dc.rights | acceso restringido | |
dc.subject | galaxies: abundances | |
dc.subject | galaxies: individual (IRAS 13120-5453) | |
dc.subject | galaxies: interactions | |
dc.subject | galaxies: starburst | |
dc.subject | radiative transfer | |
dc.subject | submillimeter: galaxies | |
dc.subject | GALACTIC CHEMICAL EVOLUTION | |
dc.subject | LUMINOUS INFRARED GALAXIES | |
dc.subject | MOLECULAR GAS | |
dc.subject | STAR-FORMATION | |
dc.subject | NGC 6240 | |
dc.subject | INTENSITY RATIOS | |
dc.subject | ARP 220 | |
dc.subject | MRK 231 | |
dc.subject | METALLICITY | |
dc.subject | (CO)-C-13 | |
dc.title | Extreme CO Isotopic Abundances in the ULIRG IRAS 13120-5453: An Extremely Young Starburst or Top-heavy Initial Mass Function | |
dc.type | artículo | |
dc.volumen | 840 | |
sipa.codpersvinculados | 1031484 | |
sipa.index | WOS | |
sipa.index | Scopus | |
sipa.trazabilidad | Carga SIPA;09-01-2024 |
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