PIRSA:09040035  ( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?

Speaker(s): Paul Bode

Abstract: "Taking gravitational potential wells from a dark matter simulation, and assuming a polytropic equation of state and hydrostatic equilibrium, one can predict the state of the hot gas in clusters of galaxies. With reasonable values for star formation efficiency, energy input, and nonthermal pressure ... read more

Date: 27/04/2009 - 2:00 pm

Collection: Sunyaev-Zeldovich Universe and the Future of Cluster Cosmology

URL: http://pirsa.org/09040035/  Share: