Multi-wavelenth monitoring of the changing-look AGN NGC 2617 during state changes
Multi-wavelenth monitoring of the changing-look AGN NGC 2617 during state changes
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Author / Creator
Oknyansky, V L , Gaskell, C M , Huseynov, N A , Mikailov, Kh M , Lipunov, V M , Shatsky, N I , Tsygankov, S S , Gorbovskoy, E S , Tatarnikov, A M , Metlov, V G , Malanchev, K L , Brotherton, M B , Kasper, D , P Du , Chen, X , Burlak, M A , Buckley, D A H , Rebolo, R , Serra-Ricart, M , Podesta, R and Levato, H
Publisher
Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Optical and near-infrared photometry, optical spectroscopy, and soft X-ray and UV monitoring of the changing-look active galactic nucleus NGC 2617 show that it continues to have the appearance of a type-1 Seyfert galaxy. An optical light curve for 2010\(-\)2017 indicates that the change of type probably occurred between 2010 October and 2012 Februa...
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Full title
Multi-wavelenth monitoring of the changing-look AGN NGC 2617 during state changes
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Record Identifier
TN_cdi_proquest_journals_2071285632
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2071285632
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1711.02631
