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X-ray emissions from clusters and groups of galaxies
Pages 72-77

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From page 72...
... clusters should retain an imprint of bag 1bey Aura armed, and thus studies of their evolution 1emper~1~re, And luminosity Unction should place strong constraints on aD tbcorTcs of large scale structure. Unlit galaxies, whim ala cc~aTn~ open Items rich clusters prawn retain all of the enriched m~1eri~1 that was created in their precollapse~ comparing volume Tllus, steadies of their chemical abtl~dallces slid its Solution should provide fundamental data far the stud of tbc mason of the elements and provide a history of ~ucleo~n1besis in the universe.
From page 73...
... ~ ~ O 1 o o Ala. Ok #} Optical velocity dip c~mpard With cm~sio~ weighted average x-~^ temperature #< a laps ssmDl~ of 1~ and high (a 0.I4)
From page 74...
... ~ n~cesssri~ includes the mass of tab smoker clusters and groups Jicb be in Ah foreground and background of the cluster Whereas the x-ray mass estimate ~ strong bided to just 1be caster i~elL ~ one as to smaller maw scam 1ban that of rich cIu$lers. the gravitational lens mass is more biased.
From page 75...
... Recent samples hosed on deeper ~osat pointed data (1. A bsvc Fund little illdic~tion of strolls cluster luminosity Unction evolution at z ~ 0.6.
From page 76...
... , , #,. 1 Dank my collaborator ~1 Goddard Space Flight Center Id on the ~C)
From page 77...
... ~ ~ ~ ~ ~ e Colloquium Paper: ~usbolz~ 2?


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