DST astronomers trace huge optical flare from supermassive black hole discovered in the 1960s
Blazars, or feeding supermassive black holes, are popular astronomical subjects due to their complicated mechanism of emission.


Illustration of a shock wave (bright blob in the upper jet) after a
spiral path (yellow) as it moves away from the black hole and through a section of
the jet where the magnetic field (light blue curved lines) is wound up in a coil. Image: Cosmovision/Instituto de Astronomia[/caption]A team of astronomers led by Alok Chandra Gupta from Aryabhatta Research Institute of Observational Sciences (ARIES), an institute of the Department of Science & Technology, who has been following the blazar since October 2020 as part of an international observational campaign detected the exceptionally high flare on January 16 with the help of Sampurnanand Telescope (ST) and 1.3 m Devasthal Fast Optical Telescopes located in Nainital.The data collected from the flare observed will help calculation of the black hole mass, size of emission region, and mechanism of the emission from one of the oldest astronomical objects known, hence opening a door to the origin and evolution of the Universe, it added.

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