The Origin of Our Solar System The Great Chain of Origins and Origin Hypotheses (Nebular Hypothesis)
The main growth modes of disks, bulges, and central black holes: Mergers - Violent Instabilities - Secular Evolution Frédéric Bournaud - CEA Saclay with.
Accretion Disks Prof. Hannah Jang-Condell. Accretion Disks Galaxy: M81 Protoplanetary Disk: AB Aurigae Neutron Star (artists conception) (Giovanni Benintende)(M.
Angular Momentum and the Formation of Stars and Black Holes Richard B. Larson Yale University.
Physics of stars Syllabus week topics ---------------------------------------------------------------------------------------------------------------------
Astrophysics Literature: zacek/zacek/ … this presentation
Dust in Dwarf Galaxies Adam Leroy N ATIONAL R ADIO A STRONOMY O BSERVATORY HERITAGE (Meixner et al.)
High Redshift Galaxies in the Great Observatories Origins Deep Survey (GOODS) Mark Dickinson (National Optical Astronomy Observatory) for the GOODS team.
Filippo Fraternali (Bologna University)3D - Munich - 12/06/08 Extra-planar gas at low and high z Extra-planar gas at low and high redshifts Filippo Fraternali.
Star Formation Why is the sunset red? The stuff between the stars Nebulae Giant molecular clouds Gravitational collapse of molecular cloud Gravitational.
Gas in the Local Group James Binney & Filippo Fraternali Oxford University.
Interactions between Galaxies Galaxy Dynamics Françoise COMBES.