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What is a protostar?

What is a protostar? Here are some definitions.

Noun
  1. (astronomy) A collection of gas and dust in space with high temperature that usually grows to the point of beginning nuclear fusion and becoming a star.
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Eventually, a protostar becomes dense enough to ignite nuclear reactions at its core, a sign that a bona fide star has been born.
As the protostar continues to collapse due to gravity, it will attract more atoms and continually increase in mass and density.
After all, the Sun was presumably once a protostar too.
Jets and outflows carry off much of the energy and angular momentum that is released as the accretion disk spirals into the central protostar.
The cloud slowly collapses due to gravity, a protostar is formed and soon the internal temperature rises high enough to ignite nuclear fusion.
It became known as the Becklin-Neugebauer object and was later determined to be the first protostar to be directly observed.

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