) at the Institut d'Astrophysique de Paris, 7-10 December 2015
Monday (07 Dec 2015)
Bahcall - Lighting up the Dark: Where is the Dark Matter?
- Old concept (Ostriker+ 1974, Davis+ 1980): M/L increases with mass scale. Larger systems are dominated by DM.
- Local M/L values (Bahcall & Kulier 2014): mass … Continue Reading ››
) at University of Edinburgh
(Day 1) 10 June 2014
Clark – The formation of Pop III stars: first collapse and early fragmentation
- (Greif+ 2011) Streaming velocities can delay Pop III star formation up to Δz ~ 4 and provide additional turbulence to the halo.
- Review of H2 and HD cooling, where HD cooling is effective when electron … Continue Reading ››
I did not attend the Monday and Tuesday talks. Here is the program
with all of the videos and slides (if provided).
Wednesday, April 16th
"Star formation in self-gravitating turbulent fluids" – Murray (CITA)