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DTSTART:20170326T010000
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DTSTART:20171029T010000
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DTSTART:20180325T010000
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DTSTART:20191027T010000
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BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20181106T114500
DTEND;TZID=Europe/Rome:20181106T124500
DTSTAMP:20260430T171240
CREATED:20180725T065755Z
LAST-MODIFIED:20180725T065755Z
UID:4164-1541504700-1541508300@www.oa-roma.inaf.it
SUMMARY:colloquium - Beate Stelzer
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-beate-stelzer/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20181106T114500
DTEND;TZID=Europe/Rome:20181106T124500
DTSTAMP:20260430T171240
CREATED:20180725T065755Z
LAST-MODIFIED:20180725T065755Z
UID:4753-1541504700-1541508300@www.oa-roma.inaf.it
SUMMARY:eROSITA: Stellar science with a new X-ray All-Sky Survey
DESCRIPTION:Nearly 30 years after ROSAT\, the german-russian mission eROSITA\, planned for\nlaunch in spring 2019\, is going to perform a new X-ray All-Sky Survey.\nThe majority of sources that will be detected with eROSITA are\nlate-type stars. I present eROSITA science cases for pre-main sequence and\nfor hydrogen-burning stars based on current studies with other\nX-ray instruments. New momentum is expected from eROSITA especially\nfor stellar population and variability studies. These comprise a wide range\nof topics including studies of the dynamics of stellar coronae (through\nflares and activity cycles)\, search for X-rays from accretion outbursts\nin young stars\, and the use of X-rays as diagnostics for\nstellar angular momentum evolution and the structure of the galactic\nstellar disk.
URL:https://www.oa-roma.inaf.it/event/colloquium-beate-stelzer-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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