Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..145m&link_type=abstract
Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista
Astronomy and Astrophysics
Astronomy
Galaxies: Dark Halos, Galaxies: Evolution, Galaxies: Star Formation
Scientific paper
We performed smooth particle hydrodynamic (SPH) simulations including star formation and self-consistent chemo-photometric evolutionary population synthesis (EPS) predictions from far-UV to 1 mm, of isolated collapsing triaxial systems. The dependence of the system evolution on some parameters so far unexplored, such as the total mass, initial geometry, dynamical state of the collapsing halo and the effects of different baryonic to dark matter (DM) mass ratios has been investigated. We find important connections between dark and luminous matter.
Curir Anna
Mazzei Paola
No associations
LandOfFree
The Star Formation Rate of Galaxies. SPH simulations of isolated triaxial collapsing systems does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Star Formation Rate of Galaxies. SPH simulations of isolated triaxial collapsing systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Star Formation Rate of Galaxies. SPH simulations of isolated triaxial collapsing systems will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1372707