Research

A multi-wavelength study of a blazar involves analyzing its emission across the electromagnetic spectrum, from radio to gamma rays, to understand its jet dynamics, particle acceleration, and radiation mechanisms. This approach helps reveal the connection between synchrotron and inverse Compton processes, shedding light on the physical conditions within the blazar's jet.

Particle acceleration in blazar jets occurs primarily through shock acceleration and magnetic reconnection, where charged particles gain energy from turbulent magnetic fields and relativistic shocks. These mechanisms drive the high-energy emission observed in blazars, producing synchrotron and inverse Compton radiation.

The study of Active Galactic Nuclei (AGN) explores the supermassive black holes at their centers, analyzing their accretion processes, jet formation, and multi-wavelength emission. Understanding AGN helps reveal their role in galaxy evolution and cosmic feedback mechanisms. Studying AGN with echo mapping.