Seminář se koná každé úterý v 10:40 v posluchárně ÚTF MFF UK
v 10. patře katedrové budovy v Tróji, V Holešovičách 2, Praha 8
Models of stellar populations rely on the distribution functions describing these being probability density functions. Models of the formation and evolution of galaxies rely on these being driven by stochastic mergers in vast numbers. I will discuss evidence which is incompatible with both notions, implying the need for very major revision of our fundamental ideas.
Jiří Horáček Jiří Bičák