Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientific paper
2012-03-15
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
14 pages, 8 tables, 5 figures, accepted for publication on MNRAS
Scientific paper
According to the now strongly supported concordance $\Lambda$CDM model, galaxies may be grossly described as a luminous component embedded in a dark matter halo. The density profile of these mass dominating haloes may be determined by N - body simulations which mimic the evolution of the tiny initial density perturbations during the process leading to the structures we observe today. Unfortunately, when the effect of baryons is taken into account, the situation gets much more complicated due to the difficulties in simulating their physics. As a consequence, a definitive prediction of how dark matter haloes should presently look like is still missing. We revisit here this issue from an observational point of view devoting our attention to dwarf galaxies. Being likely dark matter dominated, these systems are ideal candidates to investigate the present day halo density profiles and check whether dark matter related quantities correlate with the stellar ones or the environment. By fitting a large sample of well measured rotation curves, we infer constraints on both halo structural parameters (such as the logarithmic slope of the density profile and its concentration) and derived quantities (e.g., the mass fraction and the Newtonian acceleration) which could then be used to constrain galaxy formation scenarios. Moreover, we investigate whether the halo properties correlates with the environment the galaxy lives in thus offering a new tool to deepen our understanding of galaxy formation.
Cardone Vincenzo Fabrizio
Popolo Antonino Del
No associations
LandOfFree
Statistical properties of the dark matter haloes of dwarf galaxies and correlations with the environment 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 Statistical properties of the dark matter haloes of dwarf galaxies and correlations with the environment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Statistical properties of the dark matter haloes of dwarf galaxies and correlations with the environment will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-30938