BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Magnetohydrodynamic Model of the M87 Jet Based on VLBI Observation
 s
DTSTART;VALUE=DATE-TIME:20151130T145500Z
DTEND;VALUE=DATE-TIME:20151130T151500Z
DTSTAMP;VALUE=DATE-TIME:20260420T185019Z
UID:indico-contribution-44@cern.ch
DESCRIPTION:Speakers: Dr. NAKAMURA\, Masanori (ASIAA)\nM87\, possibly the 
 most studied relativistic jet in active radio galaxies\, has been spatiall
 y resolved from ten to tens of millions of Schwarzschild radii\; it gives 
 a unique opportunity for understanding an AGN jet from birth to terminatio
 n. Several key issues in AGN jets can be extensively discussed based on mu
 lti-frequency radio observations and magnetohydrodynamic (MHD) jet theorie
 s toward M87. One of our remarkable findings in M87 is the "jet break"\, a
  structural change from parabolic to conical geometry\, which coincides to
  a transition from increasing to decreasing in observed proper motions. In
  this talk\, we discuss about the jet break as a fundamental property in A
 GNs under the interplay with the SMBH growth and evolution of early-type g
 alaxies.\n\nhttps://events.mpifr-bonn.mpg.de/indico/event/4/session/1/cont
 ribution/44
LOCATION:Max-Planck-Institut für Radioastronomie\, Bonn\, Germany 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/4/session/1/contribution
 /44
END:VEVENT
END:VCALENDAR