CERN, 31 January, 2001 Egil Lillestøl, CERN & Univ. of Bergen This lecture is being recorded and will be viewable on the Web from Friday 2 nd February.
AST 5.3 PPT
Johns
Predicting neutrino mass constraints from galaxy cluster surveys
Zooming Out From Earth
Astronmy project
Earth
Chapter 15, Galaxies G alaxies come in different size and shape. In the previous chapter, we talked about how galaxies provide an environment for the stars.
1 Module 8: Clusters of Galaxies. General properties, masses and mass-to-light ratios, galaxy interactions, dynamic stability, the inter-galactic medium,
Galaxies What is a galaxy? How many stars are there in an average galaxy? About how many galaxies are there in the universe? What is the name of our galaxy?
