Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33

2); 2) ((1) Center for Physical Sciences; (2) Vilnius University Observatory; Lithuania; Lithuania); Tadas Mineikis (1; Technology; Vladas Vansevi\v{c}ius (1

arxiv: 1502.00224 · v1 · pith:5VSB3SLRnew · submitted 2015-02-01 · 🌌 astro-ph.GA

Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33

Tadas Mineikis (1 , 2) , Vladas Vansevi\v{c}ius (1 , 2) ((1) Center for Physical Sciences , Technology , Lithuania , (2) Vilnius University Observatory , Lithuania) This is my paper

classification 🌌 astro-ph.GA

keywords galaxydiskevolutionmodelstochasticsurfaceadoptingalong

0 comments

read the original abstract

We have developed a fast numerical 2-D model of galaxy disk evolution (resolved along the galaxy radius and azimuth) by adopting a scheme of parameterized stochastic self-propagating star formation. We explore the parameter space of the model and demonstrate its capability to reproduce 1-D radial profiles of the galaxy M33: gas surface density, surface brightness in the i and GALEX FUV passbands, and metallicity.

This paper has not been read by Pith yet.

Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33

discussion (0)