A Unique Event Observed
According to a study revealed within the pre-print journal arXiv, ASASSN-22ci was first detected in February 2022, showing as a typical TDE. However, a second flare was noticed 720 days later, making it one of many few documented situations of repeated TDEs.
Researchers theorise this might need resulted from a course of known as Hills seize, the place a supermassive black gap disrupts a binary star system. In such instances, one star is ejected at excessive velocity, whereas the opposite stays certain in an elongated orbit across the black gap, present process repeated tidal disruptions.
Investigating the Black Hole’s Activity
Data from ultraviolet and X-ray observations revealed the black gap chargeable for ASASSN-22ci has an estimated mass of about three million occasions that of the solar. While the star concerned in these flares doubtless has a mass just like the Sun, it stays unsure if it had a companion that escaped. Scientists consider the similarity between the 2 flares signifies that the identical star might need been disrupted twice throughout its orbit.
Looking Ahead to 2026
Researchers predict a 3rd flare may happen in early 2026 if the star survives one other shut encounter with the black gap. This anticipated occasion would supply astronomers with a uncommon alternative to look at and examine the earliest phases of a TDE in unprecedented element, shedding gentle on the mechanics of black gap interactions with stars
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