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SUMMARY:Disk formation and fragmentation during collapse of prestellar clo
 uds - Patrick Hennebelle\, CNRS\, Paris
DTSTART:20110124T160000Z
DTEND:20110124T170000Z
UID:TALK29187@talks.cam.ac.uk
CONTACT:Sijme-Jan Paardekooper
DESCRIPTION:It is well established that stars form through the collapse of
  dense cores within molecular clouds. However\, the conditions under which
  this happens\nare still the subject of intense researches. Particularly d
 ebatted is the question of the disk formation. While in purely hydrodynami
 cal cases\,\nmassive disks tend to form early and fragment quickly\, the s
 ituation appears to be more complex in the magnetized cases. Indeed\, vari
 ous teams have\nconcluded that even for modest values of the magnetic inte
 nsity\, magnetic braking is sufficiently efficient to prevent disk formati
 on. In the seminar\, I will first give an introduction to this problem and
  then review\nthe various solutions\, which have been proposed and are sti
 ll under investigation.\n
LOCATION:MR14\, DAMTP\, Pav. F
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