Tuesday, June 18, 2024

New Discovery: Massive Galactic Black Hole Awakening [Artist Animation] | ESO

New Discovery: Massive Galactic Black Hole Awakening [Artist Animation] | ESO

This animation shows the growing disc of material around the massive black hole at the center of the galaxy SDSS1335+0728. In late 2019 this galaxy suddenly started shining brighter than ever before and was classified as having an active galactic nucleus (AGN), powered by the central black hole feeding off the surrounding material.

This artist’s impression shows a ring of dark yellow clouds surrounding a brighter yellow region on a dark background, including an especially bright white dot at its center. Bright yellow, red, white, and blue stars dot the image.

Astronomers have used data from several space and ground-based observatories, including the European Southern Observatory’s Very Large Telescope (ESO’s VLT), to track how the galaxy’s brightness has varied. In a study out today, they conclude that they are witnessing changes never seen before in a galaxy—likely the result of the sudden awakening of the massive black hole at its core.

“Imagine you’ve been observing a distant galaxy for years, and it always seemed calm and inactive,” says Paula Sánchez Sáez, an astronomer at ESO in Germany and lead author of the study accepted for publication in Astronomy & Astrophysics. 

“Suddenly, its [core] starts showing dramatic changes in brightness, unlike any typical events we've seen before.” This is what happened to SDSS1335+0728, which is now classified as having an ‘active galactic nucleus’ (AGN)—a bright compact region powered by a massive black hole—after it brightened dramatically in December 2019.

Like supernova explosions or tidal disruption events—when a star gets too close to a black hole and is torn apart—it can make galaxies suddenly light up. However, these brightness variations typically last only a few dozen or, at most, a few hundreds of days. SDSS1335+0728 is still growing brighter today, more than four years after it was first seen to ‘switch on’. Moreover, the variations detected in the galaxy, located 300 million light-years away in the constellation Virgo, are unlike any seen before, pointing astronomers towards another explanation.

Massive black holes—with masses over one hundred thousand times that of our Sun—exist at the center of most galaxies, including the Milky Way. “These giant monsters usually are sleeping and not directly visible,” explains co-author Claudio Ricci, from the Diego Portales University, also in Chile. “In the case of SDSS1335+0728, we were able to observe the awakening of the massive black hole, [which] suddenly started to feast on gas available in its surroundings, becoming very bright.”

“[This] process (...) has never been observed before,” Hernández García says. Previous studies reported inactive galaxies becoming active after several years, but this is the first time the process itself—the awakening of the black hole—has been observed in real time. Ricci, who is also affiliated with the Kavli Institute for Astronomy and Astrophysics at Peking University, China, adds: “This is something that could happen also to our own Sgr A*, the massive black hole (...) located at the center of our galaxy," but it is unclear how likely this is to happen. 

Follow-up observations are still needed to rule out alternative explanations. Another possibility is that we are seeing an unusually slow tidal disruption event, or even a new phenomenon. If it is in fact a tidal disruption event, this would be the longest and faintest such event ever observed. “Regardless of the nature of the variations, [this galaxy] provides valuable information on how black holes grow and evolve,” Sánchez Sáez says. 

This research was presented in a paper entitled “SDSS1335+0728: The awakening of a ∼ 106M⊙ black hole” published in Astronomy & Astrophysics (https://aanda.org/10.1051/0004-6361/202347957).

Link: https://www.eso.org/public/archives/releases/sciencepapers/eso2409/eso2409a.pdf


Credit: ESO/M. Kornmesser

Release Date: June 18, 2024

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