Super-massive black-hole can provide clue to emission mechanism; Study Suggests

NEW DELHI: A blazar is a feeding super-massive black-hole (SMBH) in the heart of a distant galaxy that produces a high-energy jet viewed face-on from Earth. Blazars are one of the most luminous and energetic objects in the known universe with a jet composed of ionized matter traveling at nearly the speed of light directed very nearly towards an observer.

Through 153 nights, 17 scientists from 9 countries in Europe and Asia including researchers from Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, an autonomous institution of the Department of Science and Technology (DST), Government of India took 2263 image frames and observed the changes in a very high energy gamma-ray emitting blazar ‘1ES 0806+524’ using seven optical telescopes in Europe and Asia.

Dr. Ashwani Pandey, guided by Dr. Alok C. Gupta from ARIES in their study published in the Astrophysical Journal, has provided the most extensive observations of this blazar, thereby chalking out the detailed optical properties of the blazar.

The team studied in great details 1ES 0806+524’ flux, color, and spectral index variations within a day and long timescales of the blazer and explained the mechanism behind the variations.