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Massive stars are the “movers and shakers” of the interstellar medium. Their powerful feedback processes include: Radiation Jets and outflows Stellar winds HII regions Supernovae These phenomena heat gas, inject turbulence, skew stellar populations, raise galactic metallicity, and destroy molecular clouds. HST image of compact star forming region Sh 2-‐106. Credit: NASA & ESA
Massive stars are the “movers and shakers” of the interstellar medium. Their powerful feedback processes include: Radiation Jets and outflows Stellar winds HII regions Supernovae These phenomena heat gas, inject turbulence, skew stellar populations, raise galactic metallicity, and destroy molecular clouds. HST image of compact star forming region Sh 2-‐106. Credit: NASA & ESA
Page 1: Origins of Stars and their Pla
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 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.

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