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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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DTSTART:20170326T010000
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DTSTART:20171029T010000
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DTSTART:20180325T010000
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DTSTART:20190331T010000
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DTSTART:20191027T010000
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BEGIN:VEVENT
DTSTART;VALUE=DATE:20180227
DTEND;VALUE=DATE:20180228
DTSTAMP:20260429T212625
CREATED:20180220T120259Z
LAST-MODIFIED:20180220T120259Z
UID:4023-1519689600-1519775999@www.oa-roma.inaf.it
SUMMARY:Assemblea del Personale.
DESCRIPTION:RICERCATORI\, TECNICI\, AMMINISTRATIVI\, PRECARI e STRUTTURATI DELL’ INAF – OAR\n \nASSEMBLEA DEL PERSONALE\n    Martedì 27 febbraio ore 10:00\nINAF– Monte Porzio\nPer discutere di: \n1) Stabilizzazioni e Piano Fabbisogno Personale INAF 2018/2020; \n2) Contrattazione integrativa; \n3) Nuovo contratto Istruzione e Ricerca; \n4)Elezioni RSU; \n  \nSaranno presenti all’ iniziativa : \n Stefano Bernabei – Coordinatore nazionale C.d.E. INAF FLC-CGIL\nCarlo Buttarelli – Coordinatore territoriale FLC – CGIL
URL:https://www.oa-roma.inaf.it/event/assemblea-del-personale/
LOCATION:OAR Monte Porzio Catone – aula Gratton\, Via Frascati 33\, Roma\, RM\, 00136\, Italia
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20180227
DTEND;VALUE=DATE:20180228
DTSTAMP:20260429T212625
CREATED:20180220T120259Z
LAST-MODIFIED:20180220T120259Z
UID:4745-1519689600-1519775999@www.oa-roma.inaf.it
SUMMARY:Assemblea del Personale.
DESCRIPTION:RICERCATORI\, TECNICI\, AMMINISTRATIVI\, PRECARI e STRUTTURATI DELL’ INAF – OAR\n \nASSEMBLEA DEL PERSONALE\n    Martedì 27 febbraio ore 10:00\nINAF– Monte Porzio\nPer discutere di: \n1) Stabilizzazioni e Piano Fabbisogno Personale INAF 2018/2020; \n2) Contrattazione integrativa; \n3) Nuovo contratto Istruzione e Ricerca; \n4)Elezioni RSU; \n  \nSaranno presenti all’ iniziativa : \n Stefano Bernabei – Coordinatore nazionale C.d.E. INAF FLC-CGIL\nCarlo Buttarelli – Coordinatore territoriale FLC – CGIL
URL:https://www.oa-roma.inaf.it/event/assemblea-del-personale-2/
LOCATION:OAR Monte Porzio Catone – aula Gratton\, Via Frascati 33\, Roma\, RM\, 00136\, Italia
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20180227T114500
DTEND;TZID=Europe/Rome:20180227T124500
DTSTAMP:20260429T212625
CREATED:20170728T202348Z
LAST-MODIFIED:20170728T202348Z
UID:3366-1519731900-1519735500@www.oa-roma.inaf.it
SUMMARY:Bright and dustiest stars in the JWST era: powerful tools to constrain the recent star formation history
DESCRIPTION:With the advent of the JWST\, the horizon of our knowledgies will be amazingly enlarged\, providing an unprecedent look of a large volume of galaxies with a broad properties range. This will be possible in the IR domain where the extinction is low and bright cool evolved stars have their emission peak. This is the case of asymptotic giant branch stars (AGB)\, luminous objects and main dust producers for the galaxy. We present how the large release of AGB+dust evolutionary models developed in the last years\, will enable a detailed study of these sources in different systems. The distribution of these objects in the IR colour-magnitude diagrams is a powerful instrument to determine the recent star formation history of the galaxy in detail.
URL:https://www.oa-roma.inaf.it/event/seminar-by-flavia-dellagli/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20180227T114500
DTEND;TZID=Europe/Rome:20180227T124500
DTSTAMP:20260429T212625
CREATED:20170728T202348Z
LAST-MODIFIED:20170728T202348Z
UID:4720-1519731900-1519735500@www.oa-roma.inaf.it
SUMMARY:Bright and dustiest stars in the JWST era: powerful tools to constrain the recent star formation history
DESCRIPTION:With the advent of the JWST\, the horizon of our knowledgies will be amazingly enlarged\, providing an unprecedent look of a large volume of galaxies with a broad properties range. This will be possible in the IR domain where the extinction is low and bright cool evolved stars have their emission peak. This is the case of asymptotic giant branch stars (AGB)\, luminous objects and main dust producers for the galaxy. We present how the large release of AGB+dust evolutionary models developed in the last years\, will enable a detailed study of these sources in different systems. The distribution of these objects in the IR colour-magnitude diagrams is a powerful instrument to determine the recent star formation history of the galaxy in detail.
URL:https://www.oa-roma.inaf.it/event/seminar-by-flavia-dellagli-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
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