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Galaxy formation
Pages 67-71

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From page 67...
... To the commons discussed adiabatic cold dark maker (~) moms proto~l~ies Arm al relatheK low rodsb1h and rcacb bigh contrast because dley corpse ~ ~ 1~< Boor.
From page 68...
... ~ l~cr ~sdius ~ould yield a sm~ll~r vaIuc ~r :~, ~hicb in 1bis pi~1ure would be intc~reted ~s ~ cb~ractcristic rp~h ~r ~c ~semb} of ~e ~e~ded da~ b~o~ of ~lr~ ~al~ies. ~ subst~ntia~[ly smal~ler ~a~l~e ~r '> would ~probc tbe baryo~-dominat~d p=~ of g~^ie~ ~h~b ce~ai~ ~n b~b~e di~tly ~om 1be CO~ 1bat 1s ~ssumed 10 dominate clu~lers and tbe outer p~rls of indRidual spiral~ Th~ scaling picture ~ould ~iI ~ thc mass concentration ~ilbin 1h~ {eD radius of a [lusler tvpic~l~ were ~volvIn~ on , , ~ 1he scale of the Hubblc dme, but tbis is incons~tont wi1b tbe evld~cc 1b~1 cluslers are close to dramical equiJbrium al 1he {e~ radius.
From page 69...
... be Cosmic Background Explorer measurement of tab lar~escale CBR anisotr~py shaded that tE n = l the disbar peer lag index has to ~ he aged to ~ ~ I to avoid unacceptable s~ll~ll~sc,~lc Bless :Flucto~ttio~ns. Tilt als<~> its possible find surely equally socials acceptable in the Locurv~1ur~ case; s value ~ -~5 Aces a Sole 31 to the OBR Uncle fluctuations And the lame scale mass distribution.
From page 70...
... le second mammal. Tile adi~alic Add isocurvature models 1llus Might give similar ~COU~ll~tS of tube ~ Rosa am w..
From page 71...
... . palaces aslrre~ular mass concentrations ~t~dsb7ft: ~ 10.


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