The Connection between the Radio Jet and the γ-ray Emission in the Radio Galaxy 3C 120 and the Blazar CTA 102

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dc.contributor Aalto-yliopisto fi
dc.contributor Aalto University en
dc.contributor.author Casadio, Carolina
dc.contributor.author Gómez, José
dc.contributor.author Jorstad, Svetlana G.
dc.contributor.author Marscher, Alan P.
dc.contributor.author Grandi, Paola
dc.contributor.author Larionov, Valeri M.
dc.contributor.author Lister, Matthew
dc.contributor.author Smith, Paul S.
dc.contributor.author Gurwell, Mark A.
dc.contributor.author Lähteenmäki, Anne
dc.contributor.author Agudo, Iván
dc.contributor.author Molina, Sol N.
dc.contributor.author Bala, Vishal
dc.contributor.author Joshi, Manasvita
dc.contributor.author Taylor, Brian
dc.contributor.author Williamson, Karen E.
dc.contributor.author Kovalev, Yuri
dc.contributor.author Savolainen, Tuomas
dc.contributor.author Pushkarev, Alexander B.
dc.contributor.author Arkharov, Arkady A.
dc.contributor.author Blinov, Dmitry A.
dc.contributor.author Borman, George A.
dc.contributor.author Di Paola, Andrea
dc.contributor.author Grishina, Tatiana S.
dc.contributor.author Hagen-Thorn, Vladimir A.
dc.contributor.author Itoh, Ryosuke
dc.contributor.author Kopatskaya, Evgenia N.
dc.contributor.author Larionova, Elena G.
dc.contributor.author Larionova, Liudmila V.
dc.contributor.author Morozova, Daria
dc.contributor.author Rastorgueva-Foi, Elizaveta
dc.contributor.author Sergeev, Sergey G.
dc.contributor.author Tornikoski, Merja
dc.contributor.author Troitsky, Ivan
dc.contributor.author Thum, Clemens
dc.contributor.author Wiesemeyer, Helmut
dc.date.accessioned 2017-05-11T07:35:57Z
dc.date.available 2017-05-11T07:35:57Z
dc.date.issued 2016-09-27
dc.identifier.citation Casadio , C , Gómez , J , Jorstad , S G , Marscher , A P , Grandi , P , Larionov , V M , Lister , M , Smith , P S , Gurwell , M A , Lähteenmäki , A , Agudo , I , Molina , S N , Bala , V , Joshi , M , Taylor , B , Williamson , K E , Kovalev , Y , Savolainen , T , Pushkarev , A B , Arkharov , A A , Blinov , D A , Borman , G A , Di Paola , A , Grishina , T S , Hagen-Thorn , V A , Itoh , R , Kopatskaya , E N , Larionova , E G , Larionova , L V , Morozova , D , Rastorgueva-Foi , E , Sergeev , S G , Tornikoski , M , Troitsky , I , Thum , C & Wiesemeyer , H 2016 , ' The Connection between the Radio Jet and the γ-ray Emission in the Radio Galaxy 3C 120 and the Blazar CTA 102 ' Galaxies , vol 4 , no. 4 , 34 . DOI: 10.3390/galaxies4040034 en
dc.identifier.issn 2075-4434
dc.identifier.other PURE UUID: 619f02a7-cdd9-4ff9-9e44-d3bbba98168a
dc.identifier.other PURE ITEMURL: https://research.aalto.fi/en/publications/the-connection-between-the-radio-jet-and-the-ray-emission-in-the-radio-galaxy-3c-120-and-the-blazar-cta-102(619f02a7-cdd9-4ff9-9e44-d3bbba98168a).html
dc.identifier.other PURE LINK: http://adsabs.harvard.edu/abs/2016Galax...4...34C
dc.identifier.other PURE FILEURL: https://research.aalto.fi/files/11427459/galaxies_04_00034.pdf
dc.identifier.uri https://aaltodoc.aalto.fi/handle/123456789/25552
dc.description.abstract We present multi-wavelength studies of the radio galaxy 3C 120 and the blazar CTA 102 during unprecedented γ-ray flares for both sources. In both studies the analysis of γ-ray data has been compared with a series of 43 GHz VLBA images from the VLBA-BU-BLAZAR program, providing the necessary spatial resolution to probe the parsec scale jet evolution during the high energy events. To extend the radio dataset for 3C 120 we also used 15 GHz VLBA data from the MOJAVE sample. These two objects which represent very different classes of AGN, have similar properties during the γ-ray events. The γ-ray flares are associated with the passage of a new superluminal component through the mm VLBI core, but not all ejections of new components lead to γ-ray events. In both sources γ-ray events occurred only when the new components are moving in a direction closer to our line of sight. We locate the γ-ray dissipation zone a short distance from the radio core but outside of the broad line region, suggesting synchrotron self-Compton scattering as the probable mechanism for the γ-ray production. en
dc.format.extent 9
dc.format.mimetype application/pdf
dc.language.iso en en
dc.relation.ispartofseries Galaxies en
dc.relation.ispartofseries Volume 4, issue 4 en
dc.rights openAccess en
dc.subject.other 115 Astronomy and space science en
dc.title The Connection between the Radio Jet and the γ-ray Emission in the Radio Galaxy 3C 120 and the Blazar CTA 102 en
dc.type A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä fi
dc.description.version Peer reviewed en
dc.contributor.department Max-Planck-Institut für Radioastronomie
dc.contributor.department CSIC
dc.contributor.department Boston University
dc.contributor.department Istituto Nazionale di Astrofisica
dc.contributor.department St. Petersburg State University
dc.contributor.department Purdue University
dc.contributor.department University of Arizona
dc.contributor.department Harvard-Smithsonian Center for Astrophysics
dc.contributor.department Department of Radio Science and Engineering
dc.contributor.department Metsähovi Radio Observatory
dc.contributor.department Pulkovo Observatory
dc.contributor.department Crimean Astrophysical Observatory
dc.contributor.department INAF, Osservatorio Astronomico di Roma
dc.contributor.department Hiroshima University
dc.contributor.department Instituto de Radio Astronomia Milimétrica
dc.subject.keyword 115 Astronomy and space science
dc.identifier.urn URN:NBN:fi:aalto-201705113936
dc.identifier.doi 10.3390/galaxies4040034
dc.type.version publishedVersion


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