Wed
Bonoli
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Barred galaxies in the simulated and in the real Universe
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Rodriguez-Moncada
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On the origin of bulgeless galaxies
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Cataldi
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Redshift evolution of the dark matter haloes shapes
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COFFEE
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D´onghia
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When do disks form bars?
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Rodriguez, F
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Central galaxy alignment with the environment
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Sodre
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A photometric estimator of galaxy cluster masses
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LUNCH
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Avila-Reese
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It’s time of the ICL: how hydro-simulations help study the most
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Montenegro Taborda
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The growth of BCGs in the TNG300 simulation: dissecting the contributions from mergers and in situ star formation
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Lopes, A.
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Characterizing Hα emission in the Fornax cluster with S-PLUS
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Artale
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High-redshift Proto-clusters in IllustrisTNG
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COFFEE
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Biviano
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The dark matter density profile of clusters of galaxies
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Marin Gilabert
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The Role of Viscosity in Galaxy Clusters
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Groth
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Turbulence in Galaxy Clusters - Impact of the Hydrodynamical Scheme
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Carucci
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Hydrogen Intensity Mapping: The ultimate signal is the weakest of all
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SOCIAL DINNER
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20:00
Alto Botánico Boutique Chancay 600,
X5003EOL Córdoba
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