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dc.contributor.authorMa, Renyi
dc.contributor.author马任意
dc.date.accessioned2013-03-27T08:03:23Z
dc.date.available2013-03-27T08:03:23Z
dc.date.issued2012-06
dc.identifier.citationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2012,423(1):187-191zh_CN
dc.identifier.issn0035-8711
dc.identifier.urihttp://dx.doi.org/10.1111/j.1745-3933.2012.01263.x
dc.identifier.uriWOS:000304813500019
dc.identifier.urihttps://dspace.xmu.edu.cn/handle/2288/15385
dc.description.abstractThe correlation between radio and X-ray luminosity in the hard state of black hole X-ray binaries is important for unveiling the relation between the accretion flow and the jets. In this Letter, we have modelled the quasi-simultaneous multiband observations of a recently discovered transient X-ray source, IGR J17177-3656. It is found that the source is probably an outlier following the steep radio/X-ray correlation rather than an outlier in the transition region as suggested by Paizis et al. It is also found that the multiband spectrum can be successfully modelled by the luminous hot accretion flow (LHAF) but less likely by the advection dominated accretion flow. Our results support the point that LHAF can explain the steep radio/X-ray correlation.zh_CN
dc.description.sponsorshipNational Natural Science Foundation of China [11143003, 10833002]; Natural Science Foundation of Fujian Province of China [2011J01023]; National Basic Research Programme of China [2009CB824800]zh_CN
dc.language.isoenzh_CN
dc.publisherWILEY-BLACKWELLzh_CN
dc.subjectblack hole physicszh_CN
dc.subjectaccretion; accretion discszh_CN
dc.subjectstarszh_CN
dc.subjectwindszh_CN
dc.subjectoutflowszh_CN
dc.subjectX-rayszh_CN
dc.subjectbinarieszh_CN
dc.subjectindividualzh_CN
dc.subjectIGR J17177-3656zh_CN
dc.titleModelling the multiband spectrum of IGR J17177-3656zh_CN
dc.typeArticlezh_CN


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