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• W1596277809 startingPage "179" @default.
• W1596277809 abstract "o o o o o o o o oo o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o o Y ung stars f rm n a wide range f scales, pr ducing aggregates and clusters with vari us degrees f gravitati nal self-binding. The l se aggregates have a hierarchical structure in b th space and time that resembles interstellar turbulence, suggesting that these stars f rm in nly a few turbulent cr ssing times with p siti ns that map ut the previ us gas distributi n. Dense clusters, n the ther hand, are ften well mixed, as if self-gravitati nal m ti n has erased the initial fine structure. Nevertheless, s me f the y ungest dense clusters als sh w subclumping, s it may be that all stellar clustering is related t turbulence. S me f the densest clusters may als be triggered. The evidence f r mass segregati n f the stars inside clusters is reviewed, al ng with vari us explanati ns f r this effect. Other aspects f the the ry f cluster f rmati n are reviewed as well, including many specific pr p sals f r cluster f rmati n mechanisms. The c nditi ns f r the f rmati n f b und clusters are discussed. Critical star f rmati n efficiencies can be as l w as 10% if the gas rem val pr cess is sl w and if the stars are b rn at subvirial speeds. Envir nmental c nditi ns, particularly pressure, may affect the fracti n and masses f clusters that end up b und. Gl bular clusters may f rm like n rmal pen clusters but in c nditi ns that prevailed during the f rmati n f the hal and bulge, r in interacting and starburst galaxies t day. Vari us the ries f r the f rmati n f gl bular clusters are summarized." @default.
• W1596277809 created "2016-06-24" @default.
• W1596277809 creator A5034838591 @default.
• W1596277809 creator A5044106308 @default.
• W1596277809 creator A5046820264 @default.
• W1596277809 creator A5055513962 @default.
• W1596277809 date "2000-05-01" @default.
• W1596277809 modified "2023-09-26" @default.
• W1596277809 title "Observations and Theory of Star Cluster Formation" @default.
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