BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Erlangen Centre for Astroparticle Physics - ECPv6.2.3.2//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Erlangen Centre for Astroparticle Physics
X-ORIGINAL-URL:https://ecap.nat.fau.de
X-WR-CALDESC:Events for Erlangen Centre for Astroparticle Physics
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Berlin
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20210328T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20211031T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20210415T160000
DTEND;TZID=Europe/Berlin:20210415T170000
DTSTAMP:20260418T071816
CREATED:20210411T161812Z
LAST-MODIFIED:20210411T161812Z
UID:3397-1618502400-1618506000@ecap.nat.fau.de
SUMMARY:ECAP mini-series Exploring Gravity: Frank Eisenhauer
DESCRIPTION:Infrared Interferometry of the Galactic Center Black Hole\nThe Galactic Center harbors the nearest massive black hole. With a distance of only 8 kpc\, it is the closest laboratory to study the astrophysical processes at work in these extreme objects\, and to probe Einstein’s general theory of relativity in the regime of strong gravity. Our presentation gives an overview of the GRAVITY infrared interferometry observations leading to the detection of the gravitational redshift and the Schwarzschild precession in the orbit of a star orbiting the black hole in a 16 yr orbit\, and the observations of orbital motion of hot gas close to the innermost stable orbit. We further present the perspective for future measurements of the spin and quadrupole of the black hole by combining infrared interferometry and spectroscopy form extremely large telescopes\, which will then also test the cosmic censorship and no hair theorem of black holes.
URL:https://ecap.nat.fau.de/index.php/event/ecap-mini-series-exploring-gravity-frank-eisenhauer/
LOCATION:Zoom
END:VEVENT
END:VCALENDAR