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Astrophysical implications of the fermionic dark matter in galaxies
2017The main aim of this thesis is to use a fermionic dark matter (DM) model (the Ruffini-Arg\"uelles-Rueda (RAR) model) to describe the distribution of dark matter in galactic halos as an astrophysical probe of the fermionic nature of dark matter. My thesis work focuses then on testing possible effects that are caused by DM (and modeled by the RAR model ...
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Cosmology and Astrophysics From Relaxed Galaxy Clusters – II. Cosmological Constraints
Monthly Notices of the Royal Astronomical Society, 2014Anja von der Linden +2 more
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Properties of Galaxies Reproduced by a Hydrodynamic Simulation
Nature, 2014Simeon Bird +2 more
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The Formation of Submillimetre-Bright Galaxies From Gas Infall Over a Billion Years
Nature, 2015Robert Feldmann +2 more
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Strangulation as the Primary Mechanism for Shutting Down Star Formation in Galaxies
Nature, 2015Rachel Cochrane, Roberto Maiolino
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Bulgeless Dwarf Galaxies and Dark Matter Cores From Supernova-Driven Outflows
Nature, 2010Alyson Brooks, Chris B Brook, G Stinson
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Cross-Correlating 21 cm and Galaxy Surveys: Implications for Cosmology and Astrophysics
Monthly Notices of the Royal Astronomical Society, 2020Hamsa Padmanabhan, Adam Amara
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