Sagittarius A*, the supermassive black hole at our galaxy's center, influences the evolution of the Milky Way by its rotation speed and mass accumulation. Theories on supermassive black hole formation suggest they either grow by merging smaller black holes or by accreting surrounding gas. The energy emitted by Sag A* due to the intense conditions of infalling matter can heat or cool gas in the galaxy, impacting star formation and the distribution of elements throughout the galaxy. This research highlights the significant interplay between black holes and their host galaxies.
The rotational speed of Sagittarius A*, our Milky Way's supermassive black hole, is crucial in understanding its formation and growth through accretion of surrounding material.
Active supermassive black holes emit radiation that can influence the evolution of their host galaxies by heating gas, affecting star formation, and dispersing enriched materials.
The regions near black holes possess extreme conditions, which significantly impacts the surrounding galaxy structure and star density, particularly evident in the Milky Way.
Sag A*, despite its immense size comparable to our solar system, plays a pivotal role in shaping the dynamics and lifecycle of the Milky Way.
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