The radiation pressure barrier in massive star formation Rolf Kuiper
The radiation pressure barrier in massive star formation Rolf Kuiper
The radiation pressure barrier in massive star formation Rolf Kuiper
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Results:<br />
<strong>Rolf</strong> <strong>Kuiper</strong><br />
<strong>The</strong> 3 rd dimension:<br />
Angular momentum transport via self-gravity<br />
● Gravitational <strong>in</strong>stabilities (Toomre: 1 < Q < 2)<br />
● Mean accretion rate ~ viscous disk evolution<br />
Scientific colloquium – MPIA Fachbeirat, Heidelberg March, 24 th 2010
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