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SUMMARY:On 3D self-consistent model for quasi-stable stellar system
DTSTART;VALUE=DATE-TIME:20161011T121500Z
DTEND;VALUE=DATE-TIME:20161011T124500Z
DTSTAMP;VALUE=DATE-TIME:20260720T000840Z
UID:indico-contribution-667@cern.ch
DESCRIPTION:Speakers: Helen Barminova (NRNU MEPhI)\n3D self-consistent mod
 el is discussed which may describe the quasi-stable stellar system. Such m
 odel describes the system having the shape of oblate rotational ellipsoid.
  The common case of anisotropic "pressure" in the plane of symmetry is con
 sidered. Some aspects of quasi-relaxed states of such systems and possible
  system evolution are discussed shortly.\n\nhttps://indico.particle.mephi.
 ru/event/4/contributions/667/
LOCATION:Milan Hotel Hall of the 2nd floor
URL:https://indico.particle.mephi.ru/event/4/contributions/667/
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