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METHOD:PUBLISH
CALSCALE:GREGORIAN
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X-ORIGINAL-URL:https://ktfa.science.upjs.sk/
X-WR-CALNAME:Department of Theoretical Physics and Astrophysics
X-WR-CALDESC:Pavol Jozef Šafárik University in Košice
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-PUBLISHED-TTL:PT1H
X-MS-OLK-FORCEINSPECTOROPEN:TRUE
BEGIN:VEVENT
CLASS:PUBLIC
UID:MEC-6a79d4cd345b93dd7ddae5fbcb28ed02@ktfa.science.upjs.sk
DTSTART:20220203T123000Z
DTEND:20220203T140000Z
DTSTAMP:20220123T204300Z
CREATED:20220123
LAST-MODIFIED:20220130
PRIORITY:5
TRANSP:OPAQUE
SUMMARY:A-F variables from the TESS continuous viewing zone
DESCRIPTION:Marek Skarka\nAstronomical Institute of the Czech Academy of Sciences\nThe region of the main sequence where A and F stars are located is a transition region of various physical phenomena. This is the reason why we can often observe stars showing signs of rotation, pulsation, chemical peculiarity, binarity, etc. at the same time. To our current knowledge, some of the observed phenomena should not co-exist. I will discuss the identification and classification of the A-F variable stars near the ecliptic pole gathered by the TESS satellite and show some interesting cases.\nONLINE LINK ( https://teams.microsoft.com/l/meetup-join/19%3aef8d9658c1ce44649006efb21962985c%40thread.tacv2/1643546493656?context=%7b%22Tid%22%3a%22f5b68cf2-035b-428d-87f6-f7384161306d%22%2c%22Oid%22%3a%22ebaa6932-5b48-48fc-9f1d-6a5a0538ee17%22%7d )\n
URL:https://ktfa.science.upjs.sk/events/a-f-variables-from-the-tess-continuous-viewing-zone/
CATEGORIES:KTFA seminar
LOCATION:online
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