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Chapter and Conference Paper
Chemo-Photometric Models of Ring Galaxies
The peculiar ring galaxies are formed as a result of cosmic interaction. An intruder galaxy plunges through the center of a disk galaxy triggering radially expanding density waves on the disk. Here we present ...
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Chapter and Conference Paper
Multiwavelength Study of the NEPR Sample. The 60 μm Luminosity Function
We present the 60 μm luminosity function (LF) of the deepest complete IRAS selected sample [1] so far available, in the North Ecliptic Polar Region (NEPR). The LF here is the first step in the multi-wavelength st...
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Chapter and Conference Paper
Multiwavelength Maps of Simulations of Galaxy Formation
We performed smoothed particle hydro-dynamical simulations of isolated collapsing triaxial systems initially composed of dark matter (DM) and gas with cooling, shocks, star formation and feedback self-consiste...
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Chapter and Conference Paper
Disks Evolution in a Cosmological Framework
We investigate the bar instability in stellar disks embedded inside a dark matter halo evolving in a fully cosmological framework. We present cosmological simulations in which the role of the disk-halo mass ra...
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Chapter and Conference Paper
Bars and Dust in Multiwavelength Maps of Simulations of Galaxy Formation
Bars are a common feature in simulations of galaxy formation of isolated collapsing systems initially composed of dark matter and gas. They last until 16 Gyr, the final time of our runs. Dust seriously affects...
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Chapter and Conference Paper
Observability of Early Evolutionary Phases of Galaxies at mm Wavelengths
Several lines of evidence and theoretical arguments suggest that a large fraction of starlight is absorbed by interstellar dust and re-radiated at far-IR wavelengths, particularly during early evolutionary pha...