Short term and multi-band variability of the active nucleus of IC310 | Zendy

D. Eisenacher | Zendy; P. Colin | Zendy; S. Lombardi | Zendy; J. Sitarek | Zendy; Fabio Zandanel | Zendy; MAGIC Collaboration | Zendy; D. Paneque | Zendy; Fermi-LAT Collaboration | Zendy; Thomas Dauser | Zendy; F. Krauß | Zendy; Sven Wilbert | Zendy; M. Kadler | Zendy; R. Schulz | Zendy; J. Wilms | Zendy; U. Bach | Zendy; E. Ros | Zendy

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Short term and multi-band variability of the active nucleus of IC310

Author(s) -

D. Eisenacher,

P. Colin,

S. Lombardi,

J. Sitarek,

Fabio Zandanel,

MAGIC Collaboration,

D. Paneque,

Fermi-LAT Collaboration,

Thomas Dauser,

F. Krauß,

Sven Wilbert,

M. Kadler,

R. Schulz,

J. Wilms,

U. Bach,

E. Ros

Publication year - 2012

Publication title -

aip conference proceedings

Language(s) - English

Resource type - Conference proceedings

SCImago Journal Rank - 0.177

H-Index - 75

eISSN - 1551-7616

pISSN - 0094-243X

DOI - 10.1063/1.4772327

Subject(s) - physics , blazar , astrophysics , active galactic nucleus , astronomy , bl lac object , very long baseline array , gamma ray , galaxy , flux (metallurgy) , magic (telescope) , radio spectrum , radio galaxy , parsec , materials science , metallurgy

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.

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