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Galaxy in the constellation Hydra
NGC 2617
legacy surveys image of NGC 2617 (right) and MCG-01-22-027
During April 2013, a dramatic outburst was discovered at the core of NGC 2617, and the spectral type was found to have changed to a Seyfert 1. An increase in X-ray emission was observed, followed by an increase in ultraviolet and then infraredluminosity. This event can be modeled by X-ray radiation heating the accretion disk orbiting a supermassive black hole (SMBH) at the center of the galaxy. This was followed by emission at longer wavelengths from the heated disk. An increase in luminosity between 2010 and 2012 may have cleared away dust in the inner part of the disk prior to the outburst, allowing a clearer view and changing the Seyfert type of the galaxy. The SMBH has an estimated mass of 30.9+11.8 −8.5 million M☉.
Additional outbursts were observed from 2016 to 2018, in between deep minima.
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Further reading
Hoin, S.; et al. (December 2022), "Six Swift Observations of the CLAGN NGC 2617", The Astronomer's Telegram, 15804: 1, Bibcode:2022ATel15804....1H.