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Accès ouvert déclaré 2020 article

Testing two-component models on very high-energy gamma-ray-emitting BL Lac objects

33Citations signalées, ce qui n’est pas une note de qualité
53Institutions déclarées
17Pays d’affiliation déclarés

Rattachement africain : es, jp, it, ch, de, hr, in, br, pl, am, at, fi, bg, Afrique du Sud, us, gr, cl. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

Context. It has become evident that one-zone synchrotron self-Compton models are not always adequate for very high-energy (VHE) gamma-ray-emitting blazars. While two-component models perform better, they are difficult to constrain due to the large number of free parameters. Aims. In this work, we make a first attempt at taking into account the observational constraints from very long baseline interferometry (VLBI) data, long-term light curves (radio, optical, and X-rays), and optical polarisation to limit the parameter space for a two-component model and test whether or not it can still reproduce the observed spectral energy distribution (SED) of the blazars. Methods. We selected five TeV BL Lac objects based on the availability of VHE gamma-ray and optical polarisation data. We collected constraints for the jet parameters from VLBI observations. We evaluated the contributions of the two components to the optical flux by means of decomposition of long-term radio and optical light curves as well as modelling of the optical polarisation variability of the objects. We selected eight epochs for these five objects based on the variability observed at VHE gamma rays, for which we constructed the SEDs that we then modelled with a two-component model. Results. We found parameter sets which can reproduce the broadband SED of the sources in the framework of two-component models considering all available observational constraints from VLBI observations. Moreover, the constraints obtained from the long-term behaviour of the sources in the lower energy bands could be used to determine the region where the emission in each band originates. Finally, we attempt to use optical polarisation data to shed new light on the behaviour of the two components in the optical band. Our observationally constrained two-component model allows explanation of the entire SED from radio to VHE with two co-located emission regions.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref
Testing two-component models on very high-energy gamma-ray-emitting BL Lac objects
Date Crossref
01/08/2020
Éditeur
EDP Sciences
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

Universidad de La LagunaTokai UniversityUniversity of TriesteKyoto UniversityNippon Soken (Japan)RIKENThe University of TokyoNational Institute for AstrophysicsETH ZurichTU Dortmund UniversityUniversity of RijekaUniversity of ZagrebRuđer Bošković InstituteUniversity of OsijekUniversity of SplitSaha Institute of Nuclear PhysicsCentro Brasileiro de Pesquisas FísicasUniversidad Complutense de MadridUniversity of ŁódźUniversity of SienaUniversity of PaduaDeutsches Elektronen-Synchrotron DESYIstituto Nazionale di Fisica Nucleare, Sezione di PadovaMax Planck Institute for PhysicsInstitute for High Energy PhysicsUniversity of PisaIstituto Nazionale di Fisica Nucleare, Sezione di PisaUniversitat de BarcelonaA. Alikhanyan National LaboratoryInternational Center for Relativistic Astrophysics NetworkNational Academy of Sciences of ArmeniaCentro de Investigaciones Energéticas, Medioambientales y TecnológicasUniversität InnsbruckPort d'Informació CientíficaUniversity of WürzburgUniversity of TurkuTurku Centre for Computer ScienceUniversity of OuluUniversitat Autònoma de BarcelonaBulgarian Academy of SciencesUniversity of BolognaNorth-West UniversityOsservatorio Astronomico di PadovaIstituto di Radioastronomia di BolognaIstituto Nazionale di Fisica Nucleare, Sezione di TorinoCalifornia Institute of TechnologyAalto UniversityUniversity of CreteFoundation for Research and Technology HellasUniversity of ChileUniversity of ConcepciónHankasalmi ObservatoryInstitute of Astronomy and National Astronomical Observatory

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Astrophysics and Cosmic PhenomenaRadio Astronomy Observations and TechnologyNeutrino Physics Research

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