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Authordc.contributor.authorGe, J. X. 
Authordc.contributor.authorMardones Pérez, Diego 
Authordc.contributor.authorHe, J. H. 
Authordc.contributor.authorRawlings, Jonathan M. C. 
Authordc.contributor.authorLiu, Sheng-Yuan 
Authordc.contributor.authorLee, Jeong-Eun 
Authordc.contributor.authorTatematsu, Ken’ichi 
Authordc.contributor.authorLiu, Tie 
Authordc.contributor.authorZhu, Lei 
Authordc.contributor.authorChang, Qiang 
Authordc.contributor.authorInostroza, Natalia 
Authordc.contributor.authorFeng, S. 
Admission datedc.date.accessioned2020-07-06T22:15:20Z
Available datedc.date.available2020-07-06T22:15:20Z
Publication datedc.date.issued2020
Cita de ítemdc.identifier.citationThe Astrophysical Journal, 891:36 (13pp), 2020 March 1es_ES
Identifierdc.identifier.other10.3847/1538-4357/ab7007
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/175819
Abstractdc.description.abstractOffsets of molecular line emission peaks from continuum peaks are very common but frequently difficult to explain with a single spherical cloud chemical model. We propose that the spatial projection effects of an irregular three-dimensional (3D) cloud structure can be a solution. This work shows that the idea can be successfully applied to the Planck cold clump G224.4-0.6 by approximating it with four individual spherically symmetric cloud cores whose chemical patterns overlap with each other to produce observable line maps. With the empirical physical structures inferred from the observation data of this clump and a gas-grain chemical model, the four cores can satisfactorily reproduce its 850 mu m continuum map and the diverse peak offsets of CCS, HC3N, and N2H+ simultaneously at chemical ages of about 8 x 10(5) similar to 3 x 10(6) yr. The 3D projection effects on chemistry has the potential to explain such asymmetrical distributions of chemicals in many other molecular clouds.es_ES
Patrocinadordc.description.sponsorshipComision Nacional de Investigacion Cientifica y Tecnologica (CONICYT) CONICYT FONDECYT 3170768 "Light of West China" program of the Chinese Academy of Sciences (CAS) Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT) Basal AFB-170002 National Natural Science Foundation of China 11873086 U1631237 Yunnan Province of China 2017HC018 National Research Foundation of Korea NRF-2018R1A2B6003423 Korea Astronomy and Space Science Institute CONICYT International Networks for young researchers REDI170243 CONICYT/PCI/REDI170243 REDES190113 EACOA fellowship from the East Asia Core Observatories Association Chinese Academy of Scienceses_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherIOP Publishinges_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceAstrophysical Journales_ES
Keywordsdc.subjectAstrochemistryes_ES
Keywordsdc.subjectDense interstellar cloudses_ES
Keywordsdc.subjectInterstellar abundanceses_ES
Keywordsdc.subjectChemical abundanceses_ES
Títulodc.titleThree-dimensional Projection Effects on Chemistry in a Planck Galactic Cold Clumpes_ES
Document typedc.typeArtículo de revistaes_ES
dcterms.accessRightsdcterms.accessRightsAcceso Abierto
Catalogueruchile.catalogadorlajes_ES
Indexationuchile.indexArtículo de publicación ISI
Indexationuchile.indexArtículo de publicación SCOPUS


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile