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dc.contributor.authorXiao, Ming
dc.contributor.authorDu, Pu
dc.contributor.authorHorne, Keith D.
dc.contributor.authorHu, Chen
dc.contributor.authorLi, Yan-Rong
dc.contributor.authorHuang, Ying-Ke
dc.contributor.authorLu, Kai-Xing
dc.contributor.authorQiu, Jie
dc.contributor.authorWang, Fang
dc.contributor.authorBai, Jin-Ming
dc.contributor.authorBian, Wei-Hao
dc.contributor.authorHo, Luis C.
dc.contributor.authorYuan, Ye-Fei
dc.contributor.authorWang, Jian-Min
dc.date.accessioned2018-08-08T14:30:09Z
dc.date.available2018-08-08T14:30:09Z
dc.date.issued2018-09-10
dc.identifier.citationXiao , M , Du , P , Horne , K D , Hu , C , Li , Y-R , Huang , Y-K , Lu , K-X , Qiu , J , Wang , F , Bai , J-M , Bian , W-H , Ho , L C , Yuan , Y-F & Wang , J-M 2018 , ' Supermassive black holes with high accretion rates in active galactic nuclei. VII. Reconstruction of velocity-delay maps by maximum entropy method ' , Astrophysical Journal , vol. 864 , no. 2 , 109 . https://doi.org/10.3847/1538-4357/aad5e1en
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 255222650
dc.identifier.otherPURE UUID: 1f9d4370-75af-4ae7-a901-5f630dc0829e
dc.identifier.otherArXiv: http://arxiv.org/abs/1808.00705v1
dc.identifier.otherScopus: 85053415158
dc.identifier.otherWOS: 000443836000009
dc.identifier.urihttp://hdl.handle.net/10023/15783
dc.descriptionFunding: K.H. acknowledges support from STFC grant ST/M001296/1 and ST/R000824/1.en
dc.description.abstractAs one of a series of papers reporting on a large reverberation mapping campaign, we apply the maximum entropy method (MEM) to nine narrow-line Seyfert 1 galaxies with super-Eddington accretion rates observed during 2012–2013 for the velocity-delay maps of their Hβ and Hγ emission lines. The maps of six objects are reliably reconstructed using MEM. The maps of Hβ and Hγ emission lines of Mrk 335 indicate that the gas of its broad-line region (BLR) is infalling. For Mrk 142, its Hβ and Hγ lines show signatures of outflow. The Hβ and Hγ maps of Mrk 1044 demonstrate complex kinematics—a virialized motion accompanied by an outflow signature, and the Hβ map of IRAS F12397+3333 is consistent with a disk or a spherical shell. The Hβ maps of Mrk 486 and MCG +06-26-012 suggest the presence of inflow and outflow, respectively. These super-Eddington accretors show diverse geometry and kinematics. Brief discussions of their BLRs are provided for each individual object.
dc.format.extent13
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2018, American Astronomical Society. This work has been made available online in accordance with the publisher’s policies. This is the author created accepted version manuscript following peer review and as such may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.3847/1538-4357/aad5e1en
dc.subjectAccretion, accretion disksen
dc.subjectGalaxies: activeen
dc.subjectGalaxies: nucleien
dc.subjectGalaxies: Seyferten
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleSupermassive black holes with high accretion rates in active galactic nuclei. VII. Reconstruction of velocity-delay maps by maximum entropy methoden
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.3847/1538-4357/aad5e1
dc.description.statusPeer revieweden


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