BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Osservatorio Astronomico di Roma - ECPv6.15.20//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-ORIGINAL-URL:https://www.oa-roma.inaf.it
X-WR-CALDESC:Eventi per Osservatorio Astronomico di Roma
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Rome
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20180325T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20181028T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20190331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20191027T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20200329T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20201025T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20190115T114500
DTEND;TZID=Europe/Rome:20190115T124500
DTSTAMP:20260502T043122
CREATED:20180922T063208Z
LAST-MODIFIED:20180922T063208Z
UID:4416-1547552700-1547556300@www.oa-roma.inaf.it
SUMMARY:colloqium - Cristina Ramos Almeida
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloqium-cristina-ramos-almeida/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20190115T114500
DTEND;TZID=Europe/Rome:20190115T124500
DTSTAMP:20260502T043122
CREATED:20180922T063208Z
LAST-MODIFIED:20190108T113910Z
UID:4771-1547552700-1547556300@www.oa-roma.inaf.it
SUMMARY:An infrared and sub-mm view of AGN obscuration and feedback
DESCRIPTION:In the past 10-15 years our view of AGN has significantly evolved thanks to the combination of new observations and models. X-ray\, infrared and sub-mm data have been crucial to peer into the inner region of AGN and study the properties of the tori\, circum-nuclear disks and nuclear outflows. In this talk I will summarize our current view of nuclear obscuration in AGN\, focusing on the variations of the torus properties with gas phase. I will also present preliminary results of a new project aimed to characterize nuclear outflows in three gas phases (ionized\, coronal and molecular) in a sample of nearby type-2 quasars and study their impact in the stellar populations\, on-going star formation and molecular gas reservoirs of the galaxies.
URL:https://www.oa-roma.inaf.it/event/colloqium-cristina-ramos-almeida-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
END:VCALENDAR