Seminars & Events

Accretion ejection phenomena in accretion disks around compact object

Dr. Indranil Chattopadhyay
Aryabhatta Research Institute for observational sciencES (ARIES), India

Accretion is the best model to explain the high luminosity, spectra and timing properties of AGNs and microquasars. Accretion is supposed to be the prime reason also for the ejection of jets associated with these objects. We review the phenomenology of these objects based on observations, and discuss the likely scenario to explain these phenomena. We also discuss the limitations of our understanding about these objects.

back to the list