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Observations provide more information about the characteristics of the closest tidal disruption event

Observations provide more information about the characteristics of the closest tidal disruption event
February 1, 2024

An international group of astronomers has conducted observations of AT 2023clx, the closest tidal disruption event (TDE) to Earth. The results were published on the arXiv pre-print server on January 22. These findings shed light on the properties of this particular TDE. TDEs occur when a star gets too close to a supermassive black hole and is torn apart by its tidal forces. This disruption leads to the release of radiation from the accreting debris, indicating the presence of a TDE.

AT 2023clx is located in the nucleus of the galaxy NGC 3799, around 155.8 million light years away from Earth. It was initially spotted as a transient in 2014 and was identified as a TDE in July 2023. This TDE is one of the faintest known events, with a maximum blackbody luminosity of 4.56 tredecillion erg/s. Little was known about its properties due to its recent discovery, which prompted a group of astronomers led by Panos Charalampopoulos of the University of Turku in Finland to conduct a comprehensive study of AT 2023clx across various wavelengths.

The observations revealed that AT 2023clx had a peak absolute magnitude of −18.25 mag in the g-band and a maximum bolometric luminosity of 32.4 tredecillion erg/s, making it an intermediate luminosity TDE. The mass of the supermassive black hole was estimated to be around 1 million solar masses. It was also found that AT 2023clx reached its peak within 10.4 days, making it the fastest rising TDE known to date.

Spectroscopy indicated a blue continuum that cools slowly, along with broad Balmer and helium lines, which are typical in TDEs. Additionally, there was a sharp, narrow emission peak observed for the first time in a TDE. The researchers concluded that AT 2023clx resulted from the tidal disruption of a low-mass, small radius star, with a low central concentration, and below the critical value for full disruption. This type of disruption should show a sharper rise and a shallower decline in the light curves compared to other disruptions. The findings were detailed in a paper published on arXiv.

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