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X-WR-CALNAME:Osservatorio Astronomico di Roma
X-ORIGINAL-URL:https://www.oa-roma.inaf.it
X-WR-CALDESC:Eventi per Osservatorio Astronomico di Roma
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TZID:Europe/Rome
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TZNAME:CEST
DTSTART:20150329T010000
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TZNAME:CET
DTSTART:20151025T010000
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TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20160327T010000
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DTSTART:20161030T010000
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DTSTART:20170326T010000
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DTSTART:20171029T010000
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BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20160630T114500
DTEND;TZID=Europe/Rome:20160630T124500
DTSTAMP:20260409T143310
CREATED:20160425T070945Z
LAST-MODIFIED:20160425T070945Z
UID:1123-1467287100-1467290700@www.oa-roma.inaf.it
SUMMARY:The Milky Way bulge: chemical content\, kinematics and 3D structure
DESCRIPTION:During the last decade large observational efforts have been focused on understanding the formation and evolution of the Milky Way bulge by studying the spectroscopic and photometric properties of its stellar population over large and unexplored regions.\nThe emerging picture is substantially different from what previously thought and by far more complicated.\nI will review the results obtained by the recent surveys focusing in particular on the observational evidences concerning the Bulge chemical content\, kinematics and 3D structure.
URL:https://www.oa-roma.inaf.it/event/the-milky-way-bulge-chemical-content-kinematics-and-3d-structure/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20160630T114500
DTEND;TZID=Europe/Rome:20160630T124500
DTSTAMP:20260409T143310
CREATED:20160425T070945Z
LAST-MODIFIED:20160425T070945Z
UID:4667-1467287100-1467290700@www.oa-roma.inaf.it
SUMMARY:The Milky Way bulge: chemical content\, kinematics and 3D structure
DESCRIPTION:During the last decade large observational efforts have been focused on understanding the formation and evolution of the Milky Way bulge by studying the spectroscopic and photometric properties of its stellar population over large and unexplored regions.\nThe emerging picture is substantially different from what previously thought and by far more complicated.\nI will review the results obtained by the recent surveys focusing in particular on the observational evidences concerning the Bulge chemical content\, kinematics and 3D structure.
URL:https://www.oa-roma.inaf.it/event/the-milky-way-bulge-chemical-content-kinematics-and-3d-structure-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
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