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- W2116692947 endingPage "925" @default.
- W2116692947 startingPage "913" @default.
- W2116692947 abstract "The long-term variability of the multiwavelength blazar emission can be interpreted in terms of orientation variations of a helical, inhomogeneous, non-thermally emitting jet, possibly caused by the orbital motion of the parent black hole in a binary system (Villata & Raiteri 1999). The helical-jet model is here applied to explain the quasi-periodic radio-optical light curves and the broad-band spectral energy distributions (SEDs) of the BL Lac object AO 0235+16. Through a suitable choice of the model parameters, the helix rotation can well account for the periodicity of the main radio and optical outbursts and for the corresponding SED variability, while the interspersed minor radio events could be interpreted as due either to some local distortions of the helical structure or to other phenomena contributing to the source emission. In particular, the probable existence of flow instabilities provides a viable interpretation for the non-periodic features." @default.
- W2116692947 created "2016-06-24" @default.
- W2116692947 creator A5053651858 @default.
- W2116692947 creator A5066727741 @default.
- W2116692947 creator A5067065216 @default.
- W2116692947 date "2004-06-01" @default.
- W2116692947 modified "2023-09-26" @default.
- W2116692947 title "Helical jets in blazars - Interpretation of the multifrequency long-term variability of AO 0235+16" @default.
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