{"@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/1360004234733743232.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1093/pasj/64.2.32"}},{"identifier":{"@type":"URI","@value":"https://academic.oup.com/pasj/article-pdf/64/2/32/54690263/pasj_64_2_32.pdf"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1110.6512"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Combined Spectral and Timing Analysis of the Black Hole Candidate MAXI J1659−152, Discovered by MAXI and Swift"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>We report on X-ray spectral and timing results of a new black hole candidate (BHC), MAXI J1659$-$152, with an orbital period of 2.41 hr (shortest among BHCs) in a 2010 outburst from 65 Rossi X-ray Timing Explorer (RXTE) observations and 8 simultaneous Swift and RXTE observations. According to the definitions of the spectral states in Remillard and McClintock (2006, ARA&A, 44, 49), most of the observations have been classified into the intermediate state. All of the X-ray broadband spectra can be modeled by a multi-color disk plus a power-law with an exponential cutoff or a multi-color disk plus a Comptonization component. During the initial phase of the outburst, a high-energy cutoff was visible at 30–40 keV. The innermost radius of the disk gradually decreased by a factor of more than 3 from the onset of the outburst, and reached a constant value of 35$\\ d_{10}$cos$\\ i$$^{-1/2}$ km, where $\\ d_{10}$ is the distance in units of 10 kpc and $\\ i$ is the inclination. The type-C quasi-periodic oscillation (QPO) frequency varied from 1.6 Hz to 7.3 Hz in association with a change of the innermost radius, while the innermost radius remained constant during the type-B QPO detections at 1.6–4.1 Hz. Hence, we suggest that the origin of the type-B QPOs is different from that of type-C QPOs, the latter of which would originate from the disk truncation radius. Assuming the constant innermost radius in the latter phase of the outburst as the innermost stable circular orbit, the black hole mass in MAXI J1659$-$152 is estimated to be 3.6–8.0$\\ M_{\\odot}$ for a distance of 5.3–8.6 kpc and an inclination angle of 60$^{\\circ}$–75$^{\\circ}$.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1420282801192692736","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"00365016"},{"@type":"NRID","@value":"1000000365016"},{"@type":"NRID","@value":"9000412210324"},{"@type":"NRID","@value":"9000248219285"},{"@type":"NRID","@value":"9000411985449"}],"foaf:name":[{"@value":"Kazutaka Yamaoka"}],"jpcoar:affiliationName":[{"@value":"1Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuo-ku, Sagamihara 252-5258"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743108","@type":"Researcher","foaf:name":[{"@value":"Ryan Allured"}],"jpcoar:affiliationName":[{"@value":"2Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743104","@type":"Researcher","foaf:name":[{"@value":"Philip Kaaret"}],"jpcoar:affiliationName":[{"@value":"2Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743233","@type":"Researcher","foaf:name":[{"@value":"Jamie A. Kennea"}],"jpcoar:affiliationName":[{"@value":"3Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802, USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743239","@type":"Researcher","foaf:name":[{"@value":"Toshihiro Kawaguchi"}],"jpcoar:affiliationName":[{"@value":"4Center for Computational Sciences, University of Tsukuba, Ten-nodai, 1-1-1 Tsukuba, Ibaraki 305-8577"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743106","@type":"Researcher","foaf:name":[{"@value":"Poshak Gandhi"}],"jpcoar:affiliationName":[{"@value":"5Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshino-dai, Chuo-ku, Sagamihara 252-5210"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743237","@type":"Researcher","foaf:name":[{"@value":"Nicholai Shaposhnikov"}],"jpcoar:affiliationName":[{"@value":"6Department of Astronomy, CRESST/University of Maryland, College Park, MD 20742, USA"},{"@value":"7Goddard Space Flight Center, NASA, Astrophysics Science Division, Greenbelt MD 20771, USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743361","@type":"Researcher","foaf:name":[{"@value":"Yoshihiro Ueda"}],"jpcoar:affiliationName":[{"@value":"8Department of Astronomy, Kyoto University, Oiwake-cho, Sakyo-ku, Kyoto 606-8502"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743236","@type":"Researcher","foaf:name":[{"@value":"Satoshi Nakahira"}],"jpcoar:affiliationName":[{"@value":"9MAXI Team, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198"}]},{"@id":"https://cir.nii.ac.jp/crid/1420011926317223680","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"80291920"},{"@type":"NRID","@value":"1000080291920"},{"@type":"CINII_AUTHOR_ID","@value":"DA15782849"},{"@type":"URI","@value":"https://ci.nii.ac.jp/author/DA15782849#entity"},{"@type":"URI","@value":"https://viaf.org/viaf/NII%7CDA15782849"},{"@type":"NRID","@value":"9000277499571"},{"@type":"NRID","@value":"9000264240116"},{"@type":"NRID","@value":"9000401950316"},{"@type":"NRID","@value":"9000364782028"}],"foaf:name":[{"@value":"Taro Kotani"}],"jpcoar:affiliationName":[{"@value":"10Research Institute for Science and Engineering, Waseda University, 17 Kikui-cho, Shinjuku-ku, Tokyo 162-0044"}]},{"@id":"https://cir.nii.ac.jp/crid/1420001326208171520","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"30300891"},{"@type":"NRID","@value":"1000030300891"},{"@type":"NRID","@value":"9000018124154"},{"@type":"NRID","@value":"9000401948459"},{"@type":"NRID","@value":"9000248219283"},{"@type":"NRID","@value":"9000003537438"},{"@type":"NRID","@value":"9000270887537"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/read0105147"}],"foaf:name":[{"@value":"Hitoshi Negoro"}],"jpcoar:affiliationName":[{"@value":"11Department of Physics, Nihon University, 1-8-14 Kanda-Surugadai, Chiyoda-ku, Tokyo 101-8308"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743105","@type":"Researcher","foaf:name":[{"@value":"Ichiro Takahashi"}],"jpcoar:affiliationName":[{"@value":"1Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuo-ku, Sagamihara 252-5258"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743234","@type":"Researcher","foaf:name":[{"@value":"Atsumasa Yoshida"}],"jpcoar:affiliationName":[{"@value":"1Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuo-ku, Sagamihara 252-5258"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743235","@type":"Researcher","foaf:name":[{"@value":"Nobuyuki Kawai"}],"jpcoar:affiliationName":[{"@value":"12Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004234733743238","@type":"Researcher","foaf:name":[{"@value":"Satoshi Sugita"}],"jpcoar:affiliationName":[{"@value":"13EcoTopia Science Institute, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8603 yamaoka@phys.aoyama.ac.jp"}]}],"publication":{"publicationIdentifier":[{"@type":"EISSN","@value":"2053051X"},{"@type":"PISSN","@value":"00046264"},{"@type":"PISSN","@value":"https://id.crossref.org/issn/00046264"}],"prism:publicationName":[{"@value":"Publications of the Astronomical Society of Japan"}],"dc:publisher":[{"@value":"Oxford University Press (OUP)"}],"prism:publicationDate":"2012-04-25","prism:volume":"64","prism:number":"2","prism:startingPage":"32"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","url":[{"@id":"https://academic.oup.com/pasj/article-pdf/64/2/32/54690263/pasj_64_2_32.pdf"}],"createdAt":"2014-03-07","modifiedAt":"2023-12-21","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=High%20Energy%20Astrophysical%20Phenomena%20(astro-ph.HE)","dc:title":"High Energy Astrophysical Phenomena (astro-ph.HE)"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical 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