{"@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/1360574096526650752.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/0004-637x/818/1/6"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/818/i=1/a=6/pdf"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/818/i=1/a=6?key=crossref.4319f36c28f2c97e27d1c38b600ea35d"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/0004-637X/818/1/6"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/0004-637X/818/1/6/pdf"}}],"dc:title":[{"@value":"ON THE FATE OF UNSTABLE CIRCUMBINARY PLANETS: TATOOINE’S CLOSE ENCOUNTERS WITH A DEATH STAR"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>ABSTRACT</jats:title>\n               <jats:p>Circumbinary planets whose orbits become unstable may be ejected, accreted, or even captured by one of the stars. We quantify the relative rates of these channels, for a binary of secondary star’s mass fraction 0.1 with an orbit of 1 AU. The most common outcome is ejection, which happens ∼80% of the time. If binary systems form circumbinary planets readily and sloppily, this process may fill the Milky Way with free-floating planets. A significant fraction of the time, ∼20%, the unstable planet strikes the primary or secondary. We tracked whether a Jupiter-like planet would undergo tidal stripping events during close passages, and find that these events are rarely strong enough to capture the planet, although this may be observable via free-floating planets that are heated or spun-up by this process.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380574096526650752","@type":"Researcher","foaf:name":[{"@value":"Adam P. Sutherland"}]},{"@id":"https://cir.nii.ac.jp/crid/1380574096526650753","@type":"Researcher","foaf:name":[{"@value":"Daniel C. Fabrycky"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"0004637X"},{"@type":"EISSN","@value":"15384357"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2016-02-02","prism:volume":"818","prism:number":"1","prism:startingPage":"6"},"reviewed":"false","dc:rights":["https://iopscience.iop.org/page/copyright","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"http://stacks.iop.org/0004-637X/818/i=1/a=6/pdf"},{"@id":"http://stacks.iop.org/0004-637X/818/i=1/a=6?key=crossref.4319f36c28f2c97e27d1c38b600ea35d"},{"@id":"https://iopscience.iop.org/article/10.3847/0004-637X/818/1/6"},{"@id":"https://iopscience.iop.org/article/10.3847/0004-637X/818/1/6/pdf"}],"createdAt":"2016-02-02","modifiedAt":"2024-01-09","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050564288374475008","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Orbital evolution of a circumbinary planet in a gaseous disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002220783607040","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"THE FIRST CIRCUMBINARY PLANET FOUND BY MICROLENSING: OGLE-2007-BLG-349L(AB)c"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004233714242560","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Two new free-floating or wide-orbit planets from microlensing"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.3847/0004-637x/818/1/6"},{"@type":"CROSSREF","@value":"10.3847/0004-6256/152/5/125_references_DOI_WYymuasMInNqC5duCqmh6WkvSAK"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/201834557_references_DOI_WYymuasMInNqC5duCqmh6WkvSAK"},{"@type":"CROSSREF","@value":"10.1186/s40623-019-1064-0_references_DOI_WYymuasMInNqC5duCqmh6WkvSAK"}]}