PDF of powerpoint presentation - McMaster Origins Institute ...

ePAPER READ

DOWNLOAD ePAPER

origins.mcmaster.ca

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

START NOW

Simulating star formation on an adaptive Eulerian mesh

SINK PARTICLE

Mass

Accretion Rate

PROTOSTELLAR MODEL

Stellar Radius

Luminosity

Deuterium Mass

Evolutionary Stage

Polytropic Index

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

Simulating star formation on an adaptive Eulerian mesh SINK PARTICLE Mass Accretion Rate PROTOSTELLAR MODEL Stellar Radius Luminosity Deuterium Mass Evolutionary Stage Polytropic Index

Protostellar Model based on Offner et al. (2009), solid; compared to Hosokawa & Omukai (2009) calculations, dashed. Figures 1 and 2 from Klassen et al. (2012a)

Page 1 and 2: Origins of Stars and their Pla
Page 3 and 4: Massive stars are the “movers
Page 5: Simulating star formation on an
Page 9 and 10: Figure 1 from Klassen et al.
Page 11 and 12: Radiative Feedback in the Clust
Page 13 and 14: Mass-‐Radius Relation for a
Page 15: Column Density (g/cm 2 )
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.

PDF of powerpoint presentation - McMaster Origins Institute ...

Create successful ePaper yourself

Delete template?

Save as template?