The Repeating Flaring Activity of AO 0235+164
Published 2024-02-14AO 0235+164 is a blazar located at redshift \(z=0.94\), that is, more than \(\mathrm{6200 ~ Mpc}\) or \(2\times10^{10} ~ \text{light years}\) away from Earth. It is believed that the supermassive black hole at its center harbors more than 10 million of solar masses. An article about it by VHEGA group member Juan Escudero Pedrosa features in this monthly issue of Astronomy & Astrophysics.
Blazars are amongst the brightest objects in the universe. They are known to consist of a supermassive black hole at the center of a galaxy with a powerful jet that accelerates particles at speeds close to that of light towards us. These speeds make relativistic effects absolutely crucial to understand what we are seeing. They present periods of activity where their luminosity increases by several orders of magnitude, making them easily visible despite their distance. However, many questions remain about the exact mechanisms of emission and the particles involved.
The new article studies the emission of AO 0235+164 from a multi-wavelength perspective, gathering data from 7mm VLBI images to high-energy \(\gamma\)-rays. The article finds that emission is probably located at several parsecs away from the central black hole. It also studies its interesting x-ray behavior, proposing a model where the x-ray emission comes from a different zone located much closer to the central black hole based on the analysis of correlations, kinematic analysis of the jet, and spectral energy distribution modelling.
Link to the article: https://www.aanda.org/articles/aa/abs/2024/02/aa46885-23/aa46885-23.html