A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Short timescale photometric and polarimetric behavior of two BL Lacertae type objects
Tekijät: 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
Kustantaja: EDP SCIENCES S A
Julkaisuvuosi: 2015
Journal: Astronomy and Astrophysics
Tietokannassa oleva lehden nimi: ASTRONOMY & ASTROPHYSICS
Lehden akronyymi: ASTRON ASTROPHYS
Artikkelin numero: ARTN A68
Vuosikerta: 578
Sivujen määrä: 8
ISSN: 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.
