27-31 August 2018
LVH, Luisenstraße 58, 10117 Berlin
Europe/Berlin timezone
- tevpa2018@desy.de
Contact
Contribution Poster (A0 portrait)
LVH, Luisenstraße 58, 10117 Berlin
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Gamma-rays
Multi-wavelength correlations within the SSC one-zone model for high-peaked BL Lacs
Speakers
- Dr. Maria Magdalena GONZALEZ
- Dr. Nissim FRAIJA
Primary authors
- Dr. Maria Magdalena GONZALEZ (Instituto de Astronomía, UNAM)
Co-authors
- Dr. Nissim FRAIJA (Instituto de Astronomia, UNAM)
- Dr. Jose Andres GARCIA-GONZALEZ (IF-UNAM)
Abstract content
The SED of high-peaked BL Lacs is generally understood as a composition of synchrotron radiation in X-rays and self-synchrotron emission peaking at energies higher than MeV originated in one emission zone. Although most of the observations are well described by this model, orphan flares, lack of correlation between X-rays and gamma-rays and a broader SED in the gamma ray regime challenge the model. In this work, we study under which conditions it is possible to observe multi-wavelength correlations within the SSC scenario and if orphan flares are plausible.