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astro-ph1998
Cluster identification via Voronoi tessellation
M. Ramella, M. Nonino, W. Boschin +1
We propose an automated method for detecting galaxy clusters in imaging surveys based on the Voronoi tessellation technique. It appears very promising, expecially for its capabilit…
astro-ph1998
Towards a consistent model of the Galaxy: I. kinematic properties, star counts and microlensing observations
D. Méra, G. Chabrier, R. Schaeffer
We examine the most recent observational constraints arising from i) small-scale and large-scale Galactic dynamical properties, ii) star counts at faint magnitude and iii) microlen…
astro-ph1998
Towards a consistent model of the Galaxy: II. Derivation of the model
D. Méra, G. Chabrier, R. Schaeffer
We use the calculations derived in a previous paper (Méra, Chabrier and Schaeffer, 1997), based on observational constraints arising from star counts, microlensing experiments and…