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
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
<strong>Rolf</strong> <strong>Kuiper</strong><br />
Key features<br />
● Superior frequency dependent ray-trac<strong>in</strong>g step (ir<strong>radiation</strong>)<br />
● Fast and robust flux limited diffusion solver (dust emission)<br />
● Resolution down to 1.27 AU (~10 times higher than before)<br />
● Complete coverage of the accretion phase (10 5 … 10 6 yr) for the first time<br />
● First broad scan of the parameter space (37 simulations analyzed so far)<br />
Scientific colloquium – MPIA Fachbeirat, Heidelberg March, 24 th 2010
Change language