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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 ...

    Anna Curir, Paola Mazzei in Multiwavelength Map** of Galaxy Formation and Evolution (2005)

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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...

    Paola Mazzei, Daniela Bettoni in Multiwavelength Map** of Galaxy Formatio… (2005)

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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...

    Paola Mazzei, Anna Curir in Multiwavelength Map** of Galaxy Formation and Evolution (2005)

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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...

    Anna Curir, Paola Mazzei, Giuseppe Murante in Penetrating Bars through Masks of Cosmic Dust (2004)

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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...

    Paola Mazzei, Anna Curir in Penetrating Bars through Masks of Cosmic Dust (2004)

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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...

    Gianfranco De Zotti, Paola Mazzei in Science with Large Millimetre Arrays (1996)