A young star with a luminosity 150L⊙ outflow velocity of 30 km s−1, and a mass loss rate of M ̇ = 10−4M⊙ yr−1 Does radiation pressure play a role in driving the outflow?
"p=\\frac{\\sigma v^2 M}{cL}=3.6\\cdot 10^{-21}~Pa,"
the radiation pressure does not play a role in driving the outflow.
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