Normal Curve Area Problems involving only z (not x yet) To accompany Hawkes lesson 6.2 A few slides are from Hawkes Plus much original content by D.R.S.
Low-mass galaxies At high-redshift, cold gas effectively expelled by feedback Suppressed SF at high –z At lower z, haloes grow and feedback becomes less.
Pop III IMF Michael L. Norman Laboratory for Computational Astrophysics UC San Diego (with thanks to Andrea Ferrara & Mario Livio)
History of Ozone
Massive star feedback – from the first stars to the present
Discussions about Z effects on the Conti scenario Geneva, 1983
Stars rotate throughout the Universe
Seismology of the Sun and solar-like stars Jørgen Christensen-Dalsgaard Institut for Fysik og Astronomi, Aarhus Universitet.
Helioseismology
Problems with Bragg-Brentano diffractometer geometry Multilayer optics.
Simulation Results for SNAP
Opto-electronics
