Dr Maria Magdalena Gonzalez (Instituto de Astronomía, UNAM)Dr Nissim Fraija (Instituto de Astronomia, UNAM)
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.
Dr Maria Magdalena Gonzalez (Instituto de Astronomía, UNAM)