A stage 4 protostar may temporarily be thousands of times more luminous than the Sun.
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Q2: At the end of the Kelvin-Helmholtz contraction,
Q3: The fundamental difference between a protostar and
Q4: The evolution of a protostar slows significantly
Q5: The birth of stars is a battle
Q6: Rotation and magnetism both play key roles
Q8: Rotation causes the cocoon of dust to
Q9: Magnetic fields enhance the collapse of a
Q10: It takes about 1032 hydrogen atoms to
Q11: As a protostar evolves from stage 4
Q12: Stars evolve to the upper left along
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