Class 24 : Supermassive black holes Recap: What is a black hole? Case studies: M87. M106. MCG-6-30-15. What’s at the center of the Milky Way? The demographics.
Lecture 5PHYS1005 – 2003/4 Lecture 5: Stars as Black-bodies Objectives - to describe: Black-body radiation Wien’s Law Stefan-Boltzmann equation Effective.
Neutron Star Physics a kind of introduction Ulrich R.M.E. Geppert November 4th 2011U.R.M.E., Univ. of Zielona Gora1.
Review: The life of Stars. Variable Stars Eclipsing binaries (stars do not change physically, only their relative position changes) Nova (two stars “collaborating”
L ocating and O bserving O ptical C ounterparts to U nmodeled P ulses in Gravitational Waves LOOC UP LIGO-G070827-00-Z Dec 16, 2007 Jonah Kanner, Peter.
The full electromagnetic spectrum …. Temperature determines the main type of radiation emitted … (left to right: Compton, Chandra, Hubble, and Spitzer.
Sirius
White Dwarfs Neutron Stars Black Holes
Eclipsing Binaries
Chapter 23
S. Hubrig. Multiplicity of CP stars S. Hubrig, N. Ageorges, M. Schöller ESO/Chile.
First Stars and Reionization
