BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:An Origin of Misaligned Disks and Planetary Orbits: Angular Moment
 um Accretion in Star Formation Process
DTSTART;VALUE=DATE-TIME:20200515T075000Z
DTEND;VALUE=DATE-TIME:20200515T081000Z
DTSTAMP;VALUE=DATE-TIME:20240704T115620Z
UID:indico-contribution-43@meetings.aip.de
DESCRIPTION:Speakers: Shu-ichiro Inutsuka (Nagoya University)\nI try to ex
 plain the primordial origin of misalignment between the disk rotation and 
 host star’s rotation from the context of the disk formation. Theoretical
  and observational investigations have provided convincing evidence for th
 e formation of molecular cloud cores by the gravitational fragmentation of
  filamentary molecular clouds\, which has important implication for the or
 igin of the stellar initial mass function. On the other hand\, the size an
 d total angular momentum of a protoplanetary disk are supposed to be direc
 tly related to the rotational property of the parental molecular cloud cor
 e where the central protostar and surrounding disk are born. Our recent an
 alysis concludes that both the mass function and angular momentum distribu
 tion of molecular cloud core are the natural outcome of transonic turbulen
 ce with Kolmogorov spectrum in parental filamentary molecular clouds. The 
 implication of this identification is non-homogeneous angular momentum dis
 tribution inside a molecular cloud core. The actual angular momentum accre
 tion onto a young stellar object in the core should create misalignment of
  disk surrounding the star. We show the probability distribution of the mi
 salignment as a function of disk mass. This finding may explain the origin
  of misaligned planets created in those disks.\n\nhttps://meetings.aip.de/
 event/1/contributions/43/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://meetings.aip.de/event/1/contributions/43/
END:VEVENT
END:VCALENDAR