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Cosmic velocity fields and their interpretation
Pages 78-81

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From page 78...
... If~alaxiessreunbi~sed mass ~acers,lh~in~rr~d deDsily pamper from this testis{} = O.li ~ 0.^ gals test ~ important because it measures the thermal emit of a typical galaxy and ~ not biased ~ 1bc rare rich clusters of Palsies. 11 confirms 1ba1 1bc quiet thermal e<~o~mcnt of a typical aim ~ ~I1 constrained and ~ very different from tab ho1 thermal environment ch~r~cterL1ic on small scales in {bogy simulations.
From page 79...
... = 0.3 models 9ksI Ace group c~ndid~es ~ ~k simulations ha much bigger local velocity dispersions, including objects With bluesh~s, Ohm am got Served Or the rc~^ Jams outdo our ~ Local Oroup. The sma~ll-sc~le ' coldness" of Be galaxy dislr-il~ution is Bell known ~ alternative expressions: Be hlgb Mach numbers of the cosmic velocity Bald (8)
From page 80...
... A plot of ah 1TF inferred velocity and gravity field (~r ~ ~ (~) .~} far this subset off The walk l~l~I dots is sin in Fig 1.


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