Connecting steady emission and very high energy flaring states in blazars: the case of Mrk 421. Issue 2 (21st May 2021)

• Record Type: Journal Article
• Authors: Dmytriiev, A; Sol, H; Zech, A
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 505:Issue 2(2021)
• Page Start: 2712
• Page End: 2730
• Publication Date: 2021-05-21
• Subjects: acceleration of particles -- radiation mechanisms: non-thermal -- BL Lacertae objects: individual: Mrk 421; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stab1445
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Various attempts have been made in the literature at describing the origin and the physical mechanisms behind flaring events in blazars with radiative emission models, but detailed properties of multiwavelength (MWL) light curves still remain difficult to reproduce. We have developed a versatile radiative code, based on a time-dependent treatment of particle acceleration, escape, and radiative cooling, allowing us to test different scenarios to connect the continuous low-state emission self-consistently with that during flaring states. We consider flares as weak perturbations of the quiescent state and apply this description to the 2010 February MWL flare of Mrk 421, the brightest very high energy (VHE) flare ever detected from this archetypal blazar, focusing on interpretations with a minimum number of free parameters. A general criterion is obtained, which disfavours a one-zone model connecting low and high state under our assumptions. A two-zone model combining physically connected acceleration and emission regions yields a satisfactory interpretation of the available time-dependent MWL light curves and spectra of Mrk 421, although certain details remain difficult to reproduce. The two-zone scenario finally proposed for the complex quiescent and flaring VHE emitting region involves both Fermi-I and Fermi-II acceleration mechanisms, respectively, at the origin of the quiescent and flaring emission.