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Hierarchical Galaxy formation in the Local Universe

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There is an excellent agreement between <strong>the</strong> observations of <strong>the</strong><br />

Monoceros stellar r<strong>in</strong>g and N­body simulations of tidal<br />

disruption of a dwarf satellite <strong>in</strong> a low <strong>in</strong>cl<strong>in</strong>ated, almost circular<br />

prograde orbit. The stellar population of this stream support <strong>the</strong><br />

extra­Galactic orig<strong>in</strong> of this structure, reject<strong>in</strong>g that it is a<br />

Galactic feature.<br />

We provide evidence on <strong>the</strong> presence of <strong>in</strong>fall of <strong>the</strong> Sgr<br />

lead<strong>in</strong>g tail onto <strong>the</strong> Galactic disk. This would expla<strong>in</strong> <strong>the</strong> giant<br />

over­density discovered <strong>in</strong> Virgo.<br />

The study of tidal streams and extended disks <strong>in</strong> spiral galaxies<br />

<strong>in</strong> <strong>the</strong> <strong>Local</strong> <strong>Universe</strong> will allow to extend this research on <strong>the</strong><br />

<strong>formation</strong> of <strong>the</strong> components of spiral galaxies.

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