Protostars are young, developing stars formed from collapsing clouds of gas and dust. They are not yet undergoing nuclear fusion in their cores, making them cooler and dimmer than main sequence stars. As protostars contract, they heat up and eventually reach a point where nuclear fusion ignites, marking the transition to a main sequence star.
Not all protostars become true stars. Some protostars may not have enough mass to sustain nuclear fusion in their cores and never become true stars, instead becoming failed stars known as brown dwarfs.
Gravitational force is what causes protostars to form. Gravity pulls together gas and dust in a molecular cloud, causing it to clump and collapse, eventually leading to the formation of a protostar.
The Wikipedia article mentions CARMA-7 and HBC-1 as examples.
Protostars are difficult to observe because they are surrounded by dense clouds of gas and dust, which block their visible light from reaching us. Additionally, protostars are still forming and are often embedded within their natal clouds, making it challenging to distinguish them from the surrounding material. Their emission is often in the infrared, which can be absorbed by Earth's atmosphere.
Those are regions within molecular clouds called protostars, where gravity causes gas and dust to collapse and form a new star. As the protostar accumulates more material, its core becomes dense and hot enough for nuclear fusion to begin, marking the birth of a new star.
Protostars was created in 1971.
Protostars has 271 pages.
All stars are formed from protostars.
The ISBN of Protostars is 0-345-02393-5.
Protostars
Not all protostars become true stars. Some protostars may not have enough mass to sustain nuclear fusion in their cores and never become true stars, instead becoming failed stars known as brown dwarfs.
Protostars are the beggining of stars
small nebulae that fluctuate in brightness
Gravitational force is what causes protostars to form. Gravity pulls together gas and dust in a molecular cloud, causing it to clump and collapse, eventually leading to the formation of a protostar.
If you can see it, its a star. Protostars radiate only in the infrared.
Clouds of gas and dust, called nebulas and then form into protostars.
The Wikipedia article mentions CARMA-7 and HBC-1 as examples.