Simulating Stellar Birth and Death

Details Simulating Stellar Birth and Death Simulating Stellar Birth and Death

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990..507w&link_type=abstract

FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 507-509 (2008).

Physics

Star Formation, Hydrodynamics, Gamma-Ray Sources, Gamma-Ray Bursts, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Origin, Formation, Evolution, Age, And Star Formation

Scientific paper

Galaxy formation and stellar explosions involve nonlinear interplay of many physical processes. To study the death of stars, especially massive star core collapse event, we have developed a AMR relativistic hydro code based on ENZO. We will discuss the algorithms used. We have also extended those algorithms to Newtonian hydro and MHD to apply to galaxy formation and star formation.

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