Show simple item record

Files in this item

Thumbnail

Item metadata

dc.contributor.authorM. Fausnaugh, Michael
dc.contributor.authorM. Peterson, Bradley
dc.contributor.authorStarkey, David
dc.contributor.authorHorne, Keith
dc.contributor.authorand the AGN STORM Collaboration
dc.date.accessioned2017-12-05T12:30:06Z
dc.date.available2017-12-05T12:30:06Z
dc.date.issued2017-12-05
dc.identifier.citationM. Fausnaugh , M , M. Peterson , B , Starkey , D , Horne , K & and the AGN STORM Collaboration 2017 , Continuum reverberation mapping of AGN accretion disks . in Frontiers in Astronomy and Space Sciences . vol. 4 , 55 , Frontiers Media S.A. , Quasars At All Cosmic Epochs , Padova , Italy , 2/04/17 . https://doi.org/10.3389/fspas.2017.00055en
dc.identifier.citationconferenceen
dc.identifier.otherPURE: 252000727
dc.identifier.otherPURE UUID: 17f5f97d-ad85-4119-898a-8388a3805596
dc.identifier.otherWOS: 000428697200001
dc.identifier.urihttp://hdl.handle.net/10023/12253
dc.descriptionThis work was supported by a Presidential Fellowship awarded to MF buy the Ohio State University. NSF grant AST-1008882 and STScI Grant GO-13330 supported MF and BP. KH acknowledges support from STFC grant ST/M001296/1.en
dc.description.abstractWe show recent detections of inter-band continuum lags in three AGN (NGC 5548, NGC 2617, and MCG+08-11-011), which provide new constraints on the temperature profiles and absolute sizes of the accretion disks. We find lags larger than would be predicted for standard geometrically thin, optically thick accretion disks by factors of 2.3–3.3. For NGC 5548, the data span UV through optical/near-IR wavelengths, and we are able to discern a steeper temperature profile than the T ~ R−3/4 expected for a standard thin disk. Using a physical model, we are also able to estimate the inclinations of the disks for two objects. These results are similar to those found from gravitational microlensing of strongly lensed quasars, and provide a complementary approach for investigating the accretion disk structure in local, low luminosity AGN.
dc.format.extent6
dc.language.isoeng
dc.publisherFrontiers Media S.A.
dc.relation.ispartofFrontiers in Astronomy and Space Sciencesen
dc.rights© 2017 Fausnaugh, Peterson, Starkey, Horne and the AGN STORM Collaboration. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.en
dc.subjectAGN continuumen
dc.subjectGalaxies: activeen
dc.subjectIndividual: NGC5548, NGC2617, MCG+08-11-011en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-NDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleContinuum reverberation mapping of AGN accretion disksen
dc.typeConference itemen
dc.description.versionPublisher PDFen
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/10.3389/fspas.2017.00055


This item appears in the following Collection(s)

Show simple item record