6533b85afe1ef96bd12b8ce1
RESEARCH PRODUCT
The EVN view of the highly variable TeV active galaxy IC 310
R. SchulzKadler32 MatthiasE. RosD. Eisenacher GlawionU. BachD. ElsässerC. GrossbergerI. KreykenbohmK. MannheimC. MüllerJ. TrüstedtJ. Wilmssubject
High Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysicsdescription
Very-high-energy $\gamma$-ray observations of the active galaxy IC 310 with the MAGIC telescopes have revealed fast variability with doubling time scales of less than 4.8min. This implies that the emission region in IC 310 is smaller than 20% of the gravitational radius of the central supermassive black hole with a mass of $3\times 10^8 M_\odot$, which poses serious questions on the emission mechanism and classification of this enigmatic object. We report on the first quasi-simultaneous multi-frequency VLBI observations of IC 310 conducted with the EVN. We find a blazar-like one-sided core-jet structure on parsec scales, constraining the inclination angle to be less than $\sim 20^\circ$ but very small angles are excluded to limit the de-projected length of the large-scale radio jet.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2015-02-12 |