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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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On the physical properties ofz≈6–8 galaxies
Astronomy and Astrophysics, 2010Daniel Schaerer, Stephane De Barros
exaly
Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly
Astronomy and Astrophysics, 2010Jens Hjorth, Darach J Watson
exaly
The abundance of ultra-diffuse galaxies from groups to clusters
Astronomy and Astrophysics, 2017Henk Hoekstra +2 more
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Oxygen and nitrogen abundances in nearby galaxies
Astronomy and Astrophysics, 2004José M Vílchez
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Herschelunveils a puzzling uniformity of distant dusty galaxies
Astronomy and Astrophysics, 2010Emanuele Daddi +2 more
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Two-dimensional multi-component photometric decomposition of CALIFA galaxies
Astronomy and Astrophysics, 2017Tomás Ruiz-Lara +2 more
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