{"@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/1361137043922451712.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1126/science.1172740"}},{"identifier":{"@type":"URI","@value":"https://www.science.org/doi/pdf/10.1126/science.1172740"}}],"dc:title":[{"@value":"A Radio Pulsar/X-ray Binary Link"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>From X-ray Binary to Pulsar</jats:title>\n          <jats:p>\n            Pulsars with millisecond rotational periods are thought to originate from neutron stars in low-mass x-ray binaries that had their spin frequencies increased by long-lasting mass transfer from their companion stars. Using data from a radio pulsar survey,\n            <jats:bold>\n              Archibald\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"1411\" related-article-type=\"in-this-issue\" vol=\"324\" xlink:href=\"10.1126/science.1172740\">1411</jats:related-article>\n            , published online 21 May; see the Perspective by\n            <jats:bold>\n              <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" page=\"1396\" related-article-type=\"in-this-issue\" vol=\"324\" xlink:href=\"10.1126/science.1175012\">Kramer</jats:related-article>\n            </jats:bold>\n            ) found a neutron star in a low-mass X-ray binary that is in the process of turning into a radio millisecond pulsar. The system, which consists of a solar-like star and a 1.69-millisecond radio pulsar, has gone through a recent accretion phase, characteristic of low-mass X-ray binaries, but it shows no accretion disk anymore, confirming the evolutionary connection between millisecond radio pulsars and low-mass X-ray binaries.\n          </jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381137043922451847","@type":"Researcher","foaf:name":[{"@value":"Anne M. Archibald"}],"jpcoar:affiliationName":[{"@value":"Department of Physics, McGill University, 3600 Rue University, Montréal, Quebec, H3A 2T8, Canada."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451842","@type":"Researcher","foaf:name":[{"@value":"Ingrid H. Stairs"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia V6T 1Z1, Canada."},{"@value":"Australia Telescope National Facility, Commonwealth Scientific and Industrial Research Organisation (CSIRO), Post Office Box 76, Epping, New South Wales 1710, Australia."},{"@value":"Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail 39, Post Office Box 218, Hawthorn Vic 3122, Australia."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451843","@type":"Researcher","foaf:name":[{"@value":"Scott M. Ransom"}],"jpcoar:affiliationName":[{"@value":"National Radio Astronomy Observatory (NRAO), 520 Edgemont Road, Charlottesville, VA 22901, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451840","@type":"Researcher","foaf:name":[{"@value":"Victoria M. Kaspi"}],"jpcoar:affiliationName":[{"@value":"Department of Physics, McGill University, 3600 Rue University, Montréal, Quebec, H3A 2T8, Canada."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451846","@type":"Researcher","foaf:name":[{"@value":"Vladislav I. Kondratiev"}],"jpcoar:affiliationName":[{"@value":"National Radio Astronomy Observatory (NRAO), 520 Edgemont Road, Charlottesville, VA 22901, USA."},{"@value":"Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA."},{"@value":"Astro Space Center of the Lebedev Physical Institute, Profsoyuznaya 84/32, Moscow 117997, Russia."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451844","@type":"Researcher","foaf:name":[{"@value":"Duncan R. Lorimer"}],"jpcoar:affiliationName":[{"@value":"Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA."},{"@value":"National Radio Astronomy Observatory, Green Bank, WV 24944, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451715","@type":"Researcher","foaf:name":[{"@value":"Maura A. McLaughlin"}],"jpcoar:affiliationName":[{"@value":"Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA."},{"@value":"National Radio Astronomy Observatory, Green Bank, WV 24944, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451841","@type":"Researcher","foaf:name":[{"@value":"Jason Boyles"}],"jpcoar:affiliationName":[{"@value":"Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA."},{"@value":"National Radio Astronomy Observatory, Green Bank, WV 24944, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451719","@type":"Researcher","foaf:name":[{"@value":"Jason W. T. Hessels"}],"jpcoar:affiliationName":[{"@value":"Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, Netherlands."},{"@value":"Astronomical Institute Anton Pannekoek, University of Amsterdam, Kruislaan 403, 1098 SJ, Amsterdam, Netherlands."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451845","@type":"Researcher","foaf:name":[{"@value":"Ryan Lynch"}],"jpcoar:affiliationName":[{"@value":"Department of Astronomy, University of Virginia, Charlottesville, VA 22904–4325, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451716","@type":"Researcher","foaf:name":[{"@value":"Joeri van Leeuwen"}],"jpcoar:affiliationName":[{"@value":"Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, Netherlands."},{"@value":"Astronomical Institute Anton Pannekoek, University of Amsterdam, Kruislaan 403, 1098 SJ, Amsterdam, Netherlands."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451721","@type":"Researcher","foaf:name":[{"@value":"Mallory S. E. Roberts"}],"jpcoar:affiliationName":[{"@value":"Eureka Scientific, 2452 Delmer Street, Suite 100, Oakland, CA 94602-3017, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451714","@type":"Researcher","foaf:name":[{"@value":"Frederick Jenet"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy, University of Texas at Brownsville, 80 Fort Brown, Brownsville, TX 78520, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451718","@type":"Researcher","foaf:name":[{"@value":"David J. Champion"}],"jpcoar:affiliationName":[{"@value":"Australia Telescope National Facility, Commonwealth Scientific and Industrial Research Organisation (CSIRO), Post Office Box 76, Epping, New South Wales 1710, Australia."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451712","@type":"Researcher","foaf:name":[{"@value":"Rachel Rosen"}],"jpcoar:affiliationName":[{"@value":"National Radio Astronomy Observatory, Green Bank, WV 24944, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451713","@type":"Researcher","foaf:name":[{"@value":"Brad N. Barlow"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy, University of North Carolina at Chapel Hill, CB 3255, Phillips Hall, Chapel Hill, NC 27599–3255, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451717","@type":"Researcher","foaf:name":[{"@value":"Bart H. Dunlap"}],"jpcoar:affiliationName":[{"@value":"Department of Physics and Astronomy, University of North Carolina at Chapel Hill, CB 3255, Phillips Hall, Chapel Hill, NC 27599–3255, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1381137043922451720","@type":"Researcher","foaf:name":[{"@value":"Ronald A. Remillard"}],"jpcoar:affiliationName":[{"@value":"Massachusetts Institute of Technology Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, 37-287, Cambridge, MA 02139, USA."}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00368075"},{"@type":"EISSN","@value":"10959203"}],"prism:publicationName":[{"@value":"Science"}],"dc:publisher":[{"@value":"American Association for the Advancement of Science (AAAS)"}],"prism:publicationDate":"2009-06-12","prism:volume":"324","prism:number":"5933","prism:startingPage":"1411","prism:endingPage":"1414"},"reviewed":"false","url":[{"@id":"https://www.science.org/doi/pdf/10.1126/science.1172740"}],"createdAt":"2009-05-22","modifiedAt":"2024-01-10","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004233103987712","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"<i>NuSTAR</i> observations of rotation-powered pulsars and magnetars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285704927763968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"NuSTAR results and future plans for magnetar and rotation‐powered pulsar observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298338443836800","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Parkes “Murriyang” Search for Pulsars and Fast Transients in the Large Magellanic Cloud"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848658642724352","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Super-orbital variability of LS I +61°303 at TeV energies"}]},{"@id":"https://cir.nii.ac.jp/crid/1361412894232474368","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Observational diversity of magnetized neutron stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1361975841856868096","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Science with e-ASTROGAM"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1126/science.1172740"},{"@type":"CROSSREF","@value":"10.1017/s1743921312024027_references_DOI_7O4mNB9pUBDjKkNZAzvVWdif1He"},{"@type":"CROSSREF","@value":"10.1002/asna.201312032_references_DOI_7O4mNB9pUBDjKkNZAzvVWdif1He"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac5802_references_DOI_7O4mNB9pUBDjKkNZAzvVWdif1He"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/201527964_references_DOI_7O4mNB9pUBDjKkNZAzvVWdif1He"},{"@type":"CROSSREF","@value":"10.1088/1361-6633/ab3def_references_DOI_7O4mNB9pUBDjKkNZAzvVWdif1He"},{"@type":"CROSSREF","@value":"10.1016/j.jheap.2018.07.001_references_DOI_7O4mNB9pUBDjKkNZAzvVWdif1He"}]}