Big Bang
WE ARE MADE OF STAR DUST It all started with the Big Bang (a scientific theory) 13.7 b.y.a. Hydrogen and Helium were formed.
SUMMARY 1.Statistical equilibrium and radiative transfer in molecular (H 2 ) cloud – Derivation of physical parameters of molecular clouds 2.High-mass.
Formation of Stars and Galaxies. Introduction 1.Timeline and Big Bang.
Stellar Evolution What is the fate of the sun and other stars??
Unstructured grids for Astrophysics Gas dynamics and radiative transfer C.P. Dullemond Max Planck Institute for Astronomy Heidelberg, Germany.
The formation of stars and planets Day 3, Topic 3: Irradiated protoplanetary disks Lecture by: C.P. Dullemond.
Exploring Brown Dwarf Origins Ray Jayawardhana (University of Michigan -> University of Toronto) Subhanjoy Mohanty, Gibor Basri, Beate Stelzer, David Ardila,
Angular Momentum and the Formation of Stars and Black Holes Richard B. Larson Yale University.
Widescreen Test Pattern (16:9) Aspect Ratio Test (Should appear circular) 16x9 4x3.
ESAs Cosmic Vision David Southwood Director of Science and Robotic Exploration European Space Agency Paris, France 16 January 2009 International Year of.
THIS IS 11111 22222 33333 44444 5 5 555 HR diagram Life Cycle of Stars Geological time General Science universe 1 2 3 4 5 gravity.
