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Column Density (g/cm 2 )

Degravitation - McMaster Origins Institute

Origins brochure 2009.indd - McMaster Origins Institute - McMaster ...

Turbulence in Protoplanetary Disks - McMaster Origins Institute

The origin of life and and the search - McMaster Origins Institute

Turbulence and MHD Setup • 1000 M SUN clump • r -‐3/2 density profile • Turbulence (Burger’s spectrum, Mach 5 RMS) • Uniform B-‐field with M/Φ ~ 3.5 Designed to explore • Impact of HII region feedback in turbulent, magnetized clusters • Lifetimes of MC clumps 1 pc • Interplay of MHD and radiative feedback

Column Density (g/cm 2 )

Page 1 and 2: Origins of Stars and their Pla
Page 3 and 4: Massive stars are the “movers
Page 5 and 6: Simulating star formation on an
Page 7 and 8: Protostellar Model based on Off
Page 9 and 10: Figure 1 from Klassen et al.
Page 11 and 12: Radiative Feedback in the Clust
Page 13: Mass-‐Radius Relation for a
Page 18 and 19: Thank You Ralph Pudritz Thomas
Page 20 and 21: Figure 2 from Klassen et al.
Page 22: Figure 4 from Klassen et al.

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