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DTSTART:20160327T010000
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DTSTART:20161030T010000
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DTSTART;TZID=Europe/Rome:20170321T114500
DTEND;TZID=Europe/Rome:20170321T124500
DTSTAMP:20260429T212611
CREATED:20161009T045023Z
LAST-MODIFIED:20161009T045023Z
UID:1750-1490096700-1490100300@www.oa-roma.inaf.it
SUMMARY:Dwarf Galaxies - Fossils of Galaxy Evolution
DESCRIPTION:Dwarf galaxies are the most common type of galaxy in the Universe and\ninclude the most dark-matter-dominated objects known.  They offer\nintriguing insights into evolutionary processes at low halo masses\nand low metallicities.  Moreover\, as survivors of a once much more\nnumerous population of building blocks of larger galaxies\, they are\nkey to understanding very early star formation processes.  The Local\nGroup and particularly the Milky Way’s dwarf galaxy entourage offer\nus the unique possibility to compare in detail dwarf and Galactic\npopulations. This is an important step towards quantifying the\nmagnitude and time scales of dwarf contributions to the build-up of\nthe Milky Way and allows us to test predictions of cosmological\ntheories and hierarchical structure formation
URL:https://www.oa-roma.inaf.it/event/seminario-eva-grebel/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20170321T114500
DTEND;TZID=Europe/Rome:20170321T124500
DTSTAMP:20260429T212611
CREATED:20161009T045023Z
LAST-MODIFIED:20161009T045023Z
UID:4696-1490096700-1490100300@www.oa-roma.inaf.it
SUMMARY:Dwarf Galaxies - Fossils of Galaxy Evolution
DESCRIPTION:Dwarf galaxies are the most common type of galaxy in the Universe and\ninclude the most dark-matter-dominated objects known.  They offer\nintriguing insights into evolutionary processes at low halo masses\nand low metallicities.  Moreover\, as survivors of a once much more\nnumerous population of building blocks of larger galaxies\, they are\nkey to understanding very early star formation processes.  The Local\nGroup and particularly the Milky Way’s dwarf galaxy entourage offer\nus the unique possibility to compare in detail dwarf and Galactic\npopulations. This is an important step towards quantifying the\nmagnitude and time scales of dwarf contributions to the build-up of\nthe Milky Way and allows us to test predictions of cosmological\ntheories and hierarchical structure formation
URL:https://www.oa-roma.inaf.it/event/seminario-eva-grebel-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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