The radio delay of the exceptional 3C 454.3 outburst
M. VillataINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]C. M. RaiteriINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]M. F. AllerDepartment of Astronomy, University of Michigan, MI, USAU. BachINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]M. IbrahimovUlugh Beg Astronomical Institute, Academy of Sciences of Uzbekistan, UzbekistanY. Y. KovalevAstro Space Center of Lebedev Physical Institute, RussiaO. M. KurtanidzeAbastumani Astrophysical Observatory, GeorgiaV. M. LarionovAstronomical Institute, St.-Petersburg State University, RussiaChung‐Uk LeeKorea Astronomy and Space Science Institute, South KoreaP. LetoINAF, Istituto di Radioastronomia Sezione di Noto, ItalyA. LähteenmäkiMetsähovi Radio Observatory, Helsinki University of Technology, FinlandK. NilssonTuorla Observatory, FinlandT. PursimoNordic Optical Telescope, Roque de los Muchachos Astronomical Observatory, TF, SpainJavier RosN. SumitomoAstronomical Institute, Osaka Kyoiku University, JapanA. E. VolvachRadio Astronomy Laboratory of Crimean Astrophysical Observatory, UkraineH. D. AllerDepartment of Astronomy, University of Michigan, MI, USAAkira AraiAstronomical Institute, Osaka Kyoiku University, JapanC. S. BuemiINAF, Osservatorio Astrofisico di Catania, ItalyJ. M. ColomaVictor DoroshenkoMoscow State University, RussiaYu. S. EfimovCrimean Astrophysical Observatory (CrAO), UkraineL. FuhrmannDipartimento di Fisica e Osservatorio Astronomico, Università di Perugia, ItalyV. A. Hagen‐ThornAstronomical Institute, St.-Petersburg State University, RussiaM. KamadaAstronomical Institute, Osaka Kyoiku University, JapanM. KatsuuraAstronomical Institute, Osaka Kyoiku University, JapanT. S. KonstantinovaAstronomical Institute, St.-Petersburg State University, RussiaE. N. KopatskayaAstronomical Institute, St.-Petersburg State University, RussiaD. KotakaAstronomical Institute, Osaka Kyoiku University, JapanYu. A. KovalevAstro Space Center of Lebedev Physical Institute, RussiaM. KurosakiAstronomical Institute, Osaka Kyoiku University, JapanL. LanteriINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]L. V. LarionovaAstronomical Institute, St.-Petersburg State University, RussiaМ. Г. МингалиевSpecial Astrophysical Observatory, RussiaS. MizoguchiAstronomical Institute, Osaka Kyoiku University, JapanK. NakamuraAstronomical Institute, Osaka Kyoiku University, JapanM. G. NikolashviliAbastumani Astrophysical Observatory, GeorgiaShogo NishiyamaAstronomical Institute, Osaka Kyoiku University, JapanKunihiko SadakaneAstronomical Institute, Osaka Kyoiku University, JapanС. Г. СергеевCrimean Astrophysical Observatory (CrAO), UkraineL. A. SiguaAbastumani Astrophysical Observatory, GeorgiaA. SillanpääTuorla Observatory, FinlandR. L. SmartINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]L. O. TakaloTuorla Observatory, FinlandK. TanakaAstronomical Institute, Osaka Kyoiku University, JapanM. TornikoskiMetsähovi Radio Observatory, Helsinki University of Technology, FinlandC. TrigilioINAF, Osservatorio Astrofisico di Catania, ItalyG. UmanaINAF, Osservatorio Astrofisico di Catania, Italy
ABI
Аннотация
Context.In spring 2005 the blazar 3C 454.3 was observed in an unprecedented bright state from the near-IR to the hard X-ray frequencies. A mm outburst peaked in June–July 2005, and it was followed by a flux increase at high radio frequencies.
Темы
Идентификаторы
Цитирования и источники
Показатели — AkademScholar · Скоро