Research output: Contribution to journal › Article › peer-review
Blazar CTA 102 underwent exceptional optical and high-energy outbursts in 2012 and 2016-2017. We analyze its behaviour during these events, focusing on polarimetry as a tool that allows us to trace changes in the physical conditions and geometric configuration of the emission source close to the central black hole. We also use Fermi γ-ray data in conjunction with optical photometry in an effort to localize the origin of the outbursts.
Original language | English |
---|---|
Article number | 91 |
Number of pages | 7 |
Journal | Galaxies |
Volume | 5 |
Issue number | 4 |
DOIs | |
State | Published - 30 Nov 2017 |
ID: 16273256