ELFT HÍRADÓ

[ilka AT konkoly.hu (Kalman Belane)]

                            Meghivo
     
      az MTA Konkoly Thege Miklos Csillagaszati Kutatointezete 
                         Szeminariumara 
                        

Eloado: Peter Berczik
        Astronomical Observatory,
        Ukrainian National Academy of Sciences,
        UA-03680, Golosiiv, Kiev-127, Ukraine 

Cim: "Chemodynamical SPH Models of Dwarf Galaxy Formation."


Kivonat
The main purpose of our study is to implement the most recent 
developments of chemodynamical prescription of the stellar and 
gaseous components in galaxies and their interchanges into the widely 
applied general numerical treatment of hydrodynamics,  the Smoothed 
Particle Hydrodynamics (SPH). Numerical simulations of the complex 
gasdynamical flows are based on our own coding of the Chemo-Dynamical 
Smoothed Particle Hydrodynamical (CD-SPH) approach, which incorporates 
the effects of star formation and multiphase gas components. As a 
first application, the model is used to describe the chemical and 
photometric evolution of a typical star forming dwarf galaxy.
          
           
Idopont: 2001. aprilis 19. csutortok, 14 ora 
Helyszin: MTA Konkoly Thege Miklós Csillagaszati Kutatointezete eloadoterme
          Budapest, XII. Konkoly Thege u. 15/17.
  
                             
                                      Patkos Laszlo 
                                          s. k.