Short timescale photometric and polarimetric behavior of two BL Lacertae type objects



: Covino S, Baglio MC, Foschini L, Sandrinelli A, Tavecchio F, Treves A, Zhang H, de Almeida UB, Bonnoli G, Bottcher M, Cecconi M, D'Ammando F, di Fabrizio L, Giarrusso M, Leone F, Lindfors E, Lorenzi V, Molinari E, Paiano S, Prandini E, Raiteri CM, Stamerra A, Tagliaferri G

Publisher: EDP SCIENCES S A

: 2015

: Astronomy and Astrophysics

: ASTRONOMY & ASTROPHYSICS

: ASTRON ASTROPHYS

: ARTN A68

: 578

: 8

: 0004-6361

DOI: https://doi.org/10.1051/0004-6361/201525674


Conclusions. No simple scenario is able to satisfactorily model the very rich phenomenology exhibited in our data. Detailed numerical simulations show that the emitting region should be characterized by some symmetry, and the inclusion of turbulence for the magnetic field may constitute the missing ingredient for a more complete interpretation of the data.




Last updated on 2024-26-11 at 20:08