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It is believed that when a White Dwarf cools down it looses its glow and becomes a Black Dwarf

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Black holes are so dense that even light can't escape its gravity. If humans were to get anywhere close to a black hole we would be spaghettified.
They're formed because of the pressure of gravity causing the core to be packed densely with 0 volume.

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A neutron star is the compressed giant ball of neutrons that were left over from the supernova.

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Once a supernova is created there are two different paths it can take:
It can compress into a giant ball of neutrons called a neutron star.
Or a gigantic star that undergoes supernova can make a black hole.

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When the fuel runs out, the iron core becomes stable and no longer releases energy. Gravity forces the outer layers towards the core, causing it to bounce off and create an explosion known as a supernova.

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Nuclear fusion occurs, switching hydrogen into helium and heavier elements. As nuclear fusion happens, the radiation and forced outwards, creating a red supergiant.

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A tiny, Earth-sized, extremely hot core remains, slowly cooling. This is known as a White Dwarf.

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Once all the fuel has gone, the outside layers are ejected into space, creating a planetary nebular.

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When all the hydrogen goes, nuclear fusion will change, fusing helium together to make heavier elements. This causes the star to shrink and become even hotter and turn it blue.

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Helium will continue to form because of nuclear fusion as as long as there is hydrogen to fuel it.

When the fuel begins to run out, the core will shrink and its temperature will rise, making the excess energy radiate outwards, pushing the outside layers away from the core - this will form a red giant

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High mass star
⭐ Higher temperature
⭐ More fuel

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Average or low mass star
⭐ Lower temperature
⭐ Less fuel

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Once a protostar has become a main sequence star, there are two paths it can take:
Path A) Which is a high mass star. They contain more fuel and are a higher temperature.
Path B) These are average or low mass stars. They have less fuel and have a cooler temperature.

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Protostars are young stars, they contain a core that isn't yet hot enough to begin nuclear fusion.
Once it has gathered enough mass from its parent molecular cloud, and it's gained enough temperature and pressure, nuclear fusion happens. Then it becomes a main sequence star.

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A stellar nebulae is where stars are created.
When there is a lot of pressure pushing clouds of dust and gas together, a protostar is formed.