The nuclear reactions in a star's core burn steadily so long as the relationship between _____________ and_____________ is stable.
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Q22: Pre-main sequence stars (not protostars) on the
Q23: What istheresistanceofagastotheflowofradiation?
A) degeneracy
B) conduction
C) opacity
D) hydrostatic pressure
E)
Q24: Q25: Describe the concept of a "birth line" Q26: Energy flows by radiation or convection inside Q28: When a large gas cloud starts to Q29: Star clusters are important to the study Q30: How do low mass stars in the Q31: Before a giant molecular cloud can contract Q32: Briefly describe the pressure-temperature thermostat in stars.
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