Structure and dynamics in low density regions: galaxy-galaxy correlations inside cosmic voids
arXiv:1812.05532 · doi:10.1093/mnras/sty3443
Abstract
We compute the galaxy-galaxy correlation function of low-luminosity SDSS-DR7 galaxies inside cosmic voids identified in a volume limited sample of galaxies at . To identify voids, we use bright galaxies with . We find that structure in voids as traced by faint galaxies is mildly non-linear as compared with the general population of galaxies with similar luminosities. This implies a redshift-space correlation function with a similar shape than the real-space correlation albeit a normalization factor. The redshift space distortions of void galaxies allow to calculate pairwise velocity distributions which are consistent with an exponential model with a pairwise velocity dispersion of km/s, significantly lower than the global value of km/s. We also find that the internal structure of voids as traced by faint galaxies is independent of void environment, namely the correlation functions of galaxies residing in void-in-void or void-in-shell regions are identical within uncertainties. We have tested all our results with the semi-analytic catalogue MDPL2-\textsc{Sag} finding a suitable agreement with the observations in all topics studied.
Submitted to MNRAS, comments are welcome
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- How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
- Local and large-scale effects on the astrophysics of void-galaxies
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- Hickson-like compact groups inhabiting different environments
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