
In this article, the author examines the nature of objects at the centers of galaxies, traditionally classified as supermassive black holes. The focus is on the dwarf galaxy Hen 2–10 (also known as ESO 495–21), located 27 million light-years from Earth in the constellation Pyxis. Unlike many other galaxies where black holes consume matter, Hen 2–10 exhibits an unusual process: the supermassive black hole acts as a catalyst for active star formation. The author analyzes how the influence of such objects on the surrounding space changes our understanding of galactic evolution. The article offers a critical look at accepted astrophysical models, emphasizing that the interaction between black holes and interstellar gas can lead to the rapid birth of new stars, debunking the stereotype that black holes are solely 'eaters' of matter. This research opens new horizons in studying the mechanisms of star system formation in the early universe.
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