A direct result of a star collapsing could be the formation of a black hole. This occurs when the core of a massive star collapses under its own gravity, creating a region of space with such strong gravitational pull that not even light can escape.
When a supernova collapses suddenly, the intense gravitational forces cause the core to shrink rapidly, forcing protons and electrons to combine into neutrons. This results in the formation of a neutron star or a black hole, depending on the initial mass of the collapsing star. The collapse also releases an enormous amount of energy in the form of neutrinos and a blast wave, dispersing heavy elements and enriching the surrounding space.
When the gravity of a massive star overcomes neutron degeneracy pressure, it can result in the star collapsing further to form a black hole. This occurs when the mass of the star is above a certain threshold known as the Tolman–Oppenheimer–Volkoff limit, causing the neutron degeneracy pressure to be insufficient to support the star against gravity.
When the gas in the nebula's center stopped collapsing, it likely reached a stable equilibrium where the inward force of gravity was balanced by the outward pressure from nuclear fusion or other energy sources. This equilibrium could result in the formation of a protostar or a star, depending on the mass and composition of the gas.
The factor that determines whether a neutron star or a black hole forms after a supernova explosion is the mass of the collapsing core of the star. If the core's mass is between about 1.4 and 3 times the mass of the sun, a neutron star is formed. If the core's mass exceeds about 3 solar masses, a black hole is likely to form.
After the supernova of a red giant, remnants such as a neutron star or a black hole can form, depending on the mass of the original star. If the star was especially massive, it may also result in a supermassive black hole or a hypernova explosion.
As interstellar clouds approach the spiral arm region it helps them to begin the collapsing process and eventually form a star.
The pressure within a protostar counters gravity and prevents the star from collapsing further.
Super nova
When a supernova collapses suddenly, the intense gravitational forces cause the core to shrink rapidly, forcing protons and electrons to combine into neutrons. This results in the formation of a neutron star or a black hole, depending on the initial mass of the collapsing star. The collapse also releases an enormous amount of energy in the form of neutrinos and a blast wave, dispersing heavy elements and enriching the surrounding space.
By a Star collapsing on its self.
hydrostatic
The death of a star is called a supernova or stellar explosion. This is a catastrophic event that occurs when a star reaches the end of its life cycle and can result in the star either collapsing into a dense core (neutron star or black hole) or completely exploding.
The balance of forces that keep a star from collapsing is called hydrostatic equilibrium. This equilibrium is maintained between the inward force of gravity and the outward force generated by gas pressure within the star.
Dynamic equilibrium.
When the gravity of a massive star overcomes neutron degeneracy pressure, it can result in the star collapsing further to form a black hole. This occurs when the mass of the star is above a certain threshold known as the Tolman–Oppenheimer–Volkoff limit, causing the neutron degeneracy pressure to be insufficient to support the star against gravity.
Direct Star was created in 2010.
A lot of scientists consider this phenomenon to be the origin of Black Holes, which result in a gravity point so dense that it will suck in anything within it's range and crush it into it's component molecules.