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- catalog abstract "Dr. Ralph Pudritz discusses a relatively new theoretical picture for star formation which predicts that turbulence is the primary driver for the formation of the initial mass function (IMF) and reviews the basic ideas in this "turbulent fragmentation" picture, and then reports the results of recent 3D suimulations of dense molecular clumps carried out by Tilley and Pudritz (2004). He goes on to show new collapse simulations (that include molecular cooling) of such cores into protostellar disks.".
- catalog contributor b13140949.
- catalog contributor b13140950.
- catalog created "[2004]".
- catalog date "2004".
- catalog date "[2004]".
- catalog dateCopyrighted "[2004]".
- catalog description "Dr. Ralph Pudritz discusses a relatively new theoretical picture for star formation which predicts that turbulence is the primary driver for the formation of the initial mass function (IMF) and reviews the basic ideas in this "turbulent fragmentation" picture, and then reports the results of recent 3D suimulations of dense molecular clumps carried out by Tilley and Pudritz (2004). He goes on to show new collapse simulations (that include molecular cooling) of such cores into protostellar disks.".
- catalog description "Lecture held at Phillips Auditorium, Harvard College Observatory, March 4, 2004.".
- catalog description "VHS.".
- catalog extent "1 videocassette (70 min.) :".
- catalog isPartOf "CfA colloquium".
- catalog issued "2004".
- catalog issued "[2004]".
- catalog language "eng".
- catalog requires "VHS.".
- catalog subject "Stars Clusters.".
- catalog subject "Stars Formation.".
- catalog subject "Turbulence.".
- catalog title "The formation of star clusters [videorecording] : 3D simulations of hydrodynamic turbulence in self-gravitating gas / Ralph Pudritz.".
- catalog type "Videotapes. local".
- catalog type "image".