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dc.contributor.authorPing Chongzh_CN
dc.contributor.authorMa Ren-Yizh_CN
dc.contributor.authorLu Ju-Fuzh_CN
dc.contributor.author卢炬甫zh_CN
dc.date.accessioned2015-07-22T07:23:48Z
dc.date.available2015-07-22T07:23:48Z
dc.date.issued2013zh_CN
dc.identifier.citationCHINESE PHYSICS LETTERS, 2013,30(5)zh_CN
dc.identifier.otherWOS:000319436700051zh_CN
dc.identifier.urihttps://dspace.xmu.edu.cn/handle/2288/91904
dc.descriptionNational Basic Research Program of China [2009CB824800]; National Natural Science Foundation of China [11143003, 11233006, 11073015]; Natural Science Foundation of Fujian Province [2011J01023]zh_CN
dc.description.abstractThe dynamics of slim disk under the influence of a large-scale ordered magnetic field is investigated. The global solutions show that the radial velocity increases and the disk temperature decreases with enhancing magnetic field. The fraction of mass loss becomes smaller when the accretion rate is higher. The ratio of the jet kinetic power to disk luminosity is less than 0.1, which indirectly supports the argument that radio-loud narrow-line Seyfert 1 galaxies share similarities with blazars.zh_CN
dc.language.isoen_USzh_CN
dc.publisherIOP PUBLISHING LTDzh_CN
dc.source.urihttp://dx.doi.org/10.1088/0256-307X/30/5/059701zh_CN
dc.subjectDOMINATED ACCRETION FLOWSzh_CN
dc.subjectLINE SEYFERT 1zh_CN
dc.subjectSELF-SIMILAR SOLUTIONzh_CN
dc.subjectKERR BLACK-HOLESzh_CN
dc.subjectRADIATION PRESSUREzh_CN
dc.subjectPMN J0948+0022zh_CN
dc.subjectNEUTRON-STARzh_CN
dc.subjectGALAXIESzh_CN
dc.subjectJETSzh_CN
dc.subjectEMISSIONzh_CN
dc.titleThe Dynamical Effects of a Large-Scale Ordered Magnetic Field on Slim Diskszh_CN
dc.typeArticlezh_CN


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