If the initial interstellar cloud in star formation has a mass sufficient to form hundreds of stars, how does a single star form from it?
stars are formed in clusters.
Later they get separated. Astronomers estimate that the cluster will survive for about another 250 million years, after which it will disperse due to gravitational interactions with its galactic neighborhood.[8] from wiki pedia.*
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The interstellar cloud collapses due to gravity. As it does so, it breaks up into smaller areas, with one core emerging as the main mass that makes up a single star.
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The process of star formation begins within a molecular cloud, where gravitational forces cause regions of higher density to collapse. As the cloud collapses, it fragments into smaller clumps due to instabilities in its structure. These clumps continue to collapse under gravity, forming protostars. Eventually, one of these protostars becomes dominant, accreting most of the surrounding mass and evolving into a single star, while the others either merge with it or become smaller companion stars. This dominant protostar continues to accrete mass until it reaches a stable state, becoming a main-sequence star.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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