A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Rapid and multiband variability of the TeV bright active nucleus of the galaxy IC 310
Tekijät: Aleksie J, Antonelli LA, Antoranz P, Babic A, de Almeida UB, Barrio JA, Gonzalez JB, Bednarek W, Berger K, Bernardini E, Biland A, Blanch O, Bock RK, Boller A, Bonnefoy S, Bonnoli G, Tridon DB, Borracci F, Bretz T, Carmona E, Carosi A, Fidalgo DC, Colin P, Colombo E, Contreras JL, Cortina J, Cossio L, Covino S, Da Vela P, Dazzi F, De Angelis A, De Caneva G, Mendez CD, De Lotto B, Doert M, Dominguez A, Prester DD, Dorner D, Doro M, Eisenacher D, Elsaesser D, Farina E, Ferenc D, Fonseca MV, Font L, Fruck C, Lopez RJG, Garczarczyk M, Terrats DG, Gaug M, Giavitto G, Godinovic N, Munoz AG, Gozzini SR, Hadamek A, Hadasch D, Hafner D, Herrero A, Hose J, Hrupec D, Idec W, Kadenius V, Knoetig ML, Krahenbuhl T, Krause J, Kushida J, La Barbera A, Lelas D, Lewandowska N, Lindfors E, Lombardi S, Lopez-Coto R, Lopez M, Lopez-Oramas A, Lorenz E, Lozano I, Makariev M, Mallot K, Maneva G, Mankuzhiyil N, Mannheim K, Maraschi L, Marcote B, Mariotti M, Martiinez M, Masbou J, Mazin D, Meucci M, Miranda JM, Mirzoyan R, Moldoon J, Moralejo A, Munar-Adrover P, Nakajima D, Niedzwiecki A, Nilsson K, Nowak N, Orito R, Overkemping A, Paiano S, Palatiello M, Paneque D, Paoletti R, Paredes JM, Partini S, Persic M, Prada F, PradaMoroni PG, Prandini E, Preziuso S, Puljak I, Reichardt I, Reinthal R, Rhode W, Ribo M, Rico J, Ruegamer S, Saggion A, Saito K, Saito TY, Salvati M, Satalecka K, Scalzotto V, Scapin V, Schultz C, Schweizer T, Shore SN, Sillanpaa A, Sitarek J, Snidaric I, Sobczynska D, Spanier F, Spiro S, Stamatescu V, Stamerra A, Steinke B, Storz J, Sun S, Suric T, Takalo L, Takami H, Tavecchio F, Temnikov P, Terzic T, Tescaro D, Teshima M, Thaele J, Tibolla O, Torres DF, Toyama T, Treves A, Uellenbeck M, Vogler P, Wagner RM, Weitzel Q, Zandanel F, Zanin R, Dauser T, Fortin P, Kadler M, Krauss F, Wilbert S, Wilms J
Kustantaja: EDP SCIENCES S A
Julkaisuvuosi: 2014
Journal: Astronomy and Astrophysics
Tietokannassa oleva lehden nimi: ASTRONOMY & ASTROPHYSICS
Lehden akronyymi: ASTRON ASTROPHYS
Artikkelin numero: A91
Vuosikerta: 563
Sivujen määrä: 9
ISSN: 0004-6361
DOI: https://doi.org/10.1051/0004-6361/201321938
Conclusions. The rapid variability measured in gamma-rays and X-rays confirms the blazar-like behavior of IC310. The multi-TeV gamma-ray emission seems to originate from scales of less than 80 Schwarzschild radii (for a black hole mass of 2 x 10(8) M-circle dot) within the compact core of its FR I radio jet with orientation angle 10 degrees-38 degrees. The spectral energy distribution resembles that of an extreme blazar, albeit the luminosity is more than two orders of magnitude lower.
