Eisenacher D, Colin P, Lombardi S, Sitarek J, Zandanel F, Paneque D, Dauser T, Krauß F, Wilbert S, Kadler M, Schulz R, Wilms J, Bach U, Ros E (2012)
Publication Status: Published
Publication Type: Conference contribution
Publication year: 2012
Book Volume: 1505
Pages Range: 582-585
DOI: 10.1063/1.4772327
The MAGIC Telescopes detected the active galaxy IC 310 at very high energies (VHE, > 100 GeV) during observations of the Perseus cluster in 2009 and 2010. This source had originally been classified as a head-tail radio galaxy. By contrast, recent high-resolution radio images obtained with the VLBA reveal the blazar-like structure of IC 310 on parsec scales. This object is also investigated in terms of its variability at X-ray and gamma-ray energies. Studies of the multi-band flux variability at different time periods are presented. The spectral evolution seems to be different in the VHE gamma-ray and X-ray bands.
APA:
Eisenacher, D., Colin, P., Lombardi, S., Sitarek, J., Zandanel, F., Paneque, D.,... Ros, E. (2012). Short term and multi-band variability of the active nucleus of IC 310. (pp. 582-585).
MLA:
Eisenacher, Dorit, et al. "Short term and multi-band variability of the active nucleus of IC 310." 2012. 582-585.
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