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Almost every large galaxy has a supermassive black hole at its center. When two galaxies merge, it is possible to form a pair of black holes that orbit each other. A new study based on information from the Gemini North telescope looked at such a binary system in the elliptical galaxy B2 0402+379. In many ways, this is a standard pair.
Below are a pair of the most massive black holes
This is the only binary system of supermassive black holes that has been “separated” in such a way that both objects can be seen separately. In addition, there is the standard distance between the two holes, which is only 24 light-years, which theoretically indicates the possibility of a merger. But the pair have been stuck in their position for more than three billion years, and astronomers have long wondered what the obstacle was.
The team carefully mapped the area and calculated the mass of the described binary system Up to 28 billion solar masses. No similar configuration that could boast such a result has been found before. The Mass is also supposed to be an explanation for why the aforementioned merger never happened. As Martin Steele, NSF program director at the International Gemini Observatory, points out:
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