Aleksic J, Ansoldi S, Antonelli LA, Antoranz P, Babic A, Bangale P, Barrio JA, Becerra Gonzalez J, Bednarek W, Bernardini E, Biasuzzi B, Biland A, Blanch O, Bonnefoy S, Bonnoli G, Borracci F, Bretz T, Carmona E, Carosi A, Colin P, Colombo E, Contreras JL, Cortina J, Covino S, Da Vela P, Dazzi F, De Angelis A, De Caneva G, De Lotto B, De Ona Wilhelmi E, Delgado Mendez C, Dominis Prester D, Dorner D, Doro M, Einecke S, Eisenacher D, Elsaesser D, Fonseca MV, Font L, Frantzen K, Fruck C, Galindo D, Garcia Lopez RJ, Garczarczyk M, Garrido Terrats D, Gaug M, Godinovic N, Gonzalez Munoz A, Gozzini SR, Hadasch D, Hanabata Y, Hayashida M, Herrera J, Hildebrand D, Hose J, Hrupec D, Idec W, Kadenius V, Kellermann H, Kodani K, Konno Y, Krause J, Kubo H, Kushida J, La Barbera A, Lelas D, Lewandowska N, Lindfors E, Lombardi S, Longo F, Lopez M, Lopez-Coto R, Lopez-Oramas A, Lorenz E, Lozano I, Makariev M, Mallot K, Maneva G, Mankuzhiyil N, Mannheim K, Maraschi L, Marcote B, Mariotti M, Martinez M, Mazin D, Menzel U, Miranda JM, Mirzoyan R, Moralejo A, Munar-Adrover P, Nakajima D, Niedzwiecki A, Nilsson K, Nishijima K, Noda K, Orito R, Overkemping A, Paiano S, Palatiello M, Paneque D, Paoletti R, Paredes JM, Paredes-Fortuny X, Persic M, Poutanen J, Prada Moroni PG, Prandini E, Puljak I, Reinthal R, Rhode W, Ribo M, Rico J, Rodriguez Garcia J, Ruegamer S, Saito T, Saito K, Satalecka K, Scalzotto V, Scapin V, Schultz C, Schweizer T, Shore SN, Sillanpaa A, Sitarek J, Snidaric I, Sobczynska D, Spanier F, Stamatescu V, Stamerra A, Steinbring T, Storz J, Strzys M, 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, Zanin R, Kadler M, Schulz R, Ros E, Bach U, Krauss F, Wilms J (2014)
Publication Status: Published
Publication Type: Journal article
Publication year: 2014
Publisher: AMER ASSOC ADVANCEMENT SCIENCE
Book Volume: 346
Pages Range: 1080-1084
Journal Issue: 6213
Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescopes, revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20% of the gravitational radius of its central black hole. We suggest that the emission is associated with pulsar-like particle acceleration by the electric field across a magnetospheric gap at the base of the radio jet.
APA:
Aleksic, J., Ansoldi, S., Antonelli, L.A., Antoranz, P., Babic, A., Bangale, P.,... Wilms, J. (2014). Black hole lightning due to particle acceleration at subhorizon scales. Science, 346(6213), 1080-1084. https://doi.org/10.1126/science.1256183
MLA:
Aleksic, J., et al. "Black hole lightning due to particle acceleration at subhorizon scales." Science 346.6213 (2014): 1080-1084.
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