{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360004234385404032.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1088/0004-637x/799/2/230"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/799/i=2/a=230/pdf"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/799/i=2/a=230?key=crossref.7c3ceb22c8ee788a181c931129ed8ca0"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1412.1967"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"A NEW CHEMICAL EVOLUTION MODEL FOR DWARF SPHEROIDAL GALAXIES BASED ON OBSERVED LONG STAR FORMATION HISTORIES"}],"description":[{"notation":[{"@value":"We present a new chemical evolution model for dwarf spheroidal galaxies (dSphs) in the Local Universe. Our main aim is to explain both their observed star formation histories and metallicity distribution functions simultaneously. Applying our new model for the four local dSphs, that is, Fornax, Sculptor, Leo II, and Sextans, we find that our new model reproduces the observed chemical properties of the dSphs consistently. Our results show that the dSphs have evolved with both a low star formation efficiency and a large gas outflow efficiency compared with the Milky Way, as suggested by previous works. Comparing the observed [alpha/Fe]--[Fe/H] relation of the dSphs with the model predictions, we find that our model favors a longer onset time of Type Ia supernovae (i.e., 0.5 Gyr) than that suggested in previous studies (i.e., 0.1 Gyr). We discuss the origin of this discrepancy in detail."}]},{"notation":[{"@value":"18 pages, 13 figures, Accepted for publication in ApJ"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004234385403909","@type":"Researcher","foaf:name":[{"@value":"Hidetomo Homma"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234385403779","@type":"Researcher","foaf:name":[{"@value":"Takashi Murayama"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234385404033","@type":"Researcher","foaf:name":[{"@value":"Masakazu A. R. Kobayashi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234385403653","@type":"Researcher","foaf:name":[{"@value":"Yoshiaki Taniguchi"}]}],"publication":{"publicationIdentifier":[{"@type":"EISSN","@value":"15384357"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2015-01-30","prism:volume":"799","prism:number":"2","prism:startingPage":"230"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","dc:rights":["http://iopscience.iop.org/info/page/text-and-data-mining","http://iopscience.iop.org/page/copyright"],"url":[{"@id":"http://stacks.iop.org/0004-637X/799/i=2/a=230/pdf"},{"@id":"http://stacks.iop.org/0004-637X/799/i=2/a=230?key=crossref.7c3ceb22c8ee788a181c931129ed8ca0"}],"createdAt":"2015-01-30","modifiedAt":"2020-11-06","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20of%20Galaxies%20(astro-ph.GA)","dc:title":"Astrophysics of Galaxies (astro-ph.GA)"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Astrophysics%20of%20Galaxies","dc:title":"Astrophysics - Astrophysics of Galaxies"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040282257121056128","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"23244031"},{"@type":"JGN","@value":"JP23244031"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-23244031/"}],"notation":[{"@language":"ja","@value":"ウルトラ・ビスタによる初代銀河と宇宙再電離の観測的研究"},{"@language":"en","@value":"Observational Study of both Forming Galaxies and Cosmic Reionization by UltraVISTA"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004239675002752","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Metallicity Distribution of Disk Stars and the Formation History of the Milky Way"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143682023808","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Star Formation in the Milky Way and Nearby Galaxies"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143711528064","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Detailed chemical evolution of Carina and Sagittarius dwarf spheroidal galaxies"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144085807872","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE ACS NEARBY GALAXY SURVEY TREASURY. 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