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Cool gas evolution

Ken Kovacs

Word about the elements particles of the early years of the universe.      This allowed galaxies to merge and grow.          Chemical signatures of heavy elements  form primordial gases of hydrogen & helium gases.

 ABCDEFGHIJKLMNOPQR
1ledgildsmoothlygen
2eistnemelerutangis
3oantcasvvsamriddle
4anderrboselcgdimwi
5bczleuflvalrorsaex
6eicvatcueneotorpsa
7seirsyrtbmtepmliul
8tnemeleiuascailuca
9utgadtgohrrugrnlkg
10llmihginitehhplgis
11galaxyoointsgbaynr
12aflntrdnndnndicoga
13stdmrewritinglinte
14eeeeotrtotclslmahy
15srfirstiagfrlieiav
16tnuhiyttaneiaohwla
17heliumosglbnhncese
18tsloeruoxdiscskemh
accretionafteralmost
ancientbangbig
billionbillionschemical
collidingcoolcrank
developingdiscsearly
elementelementsevolution
firstfuelgalaxies
galaxygasgases
heavyheliumhunt
hydrogeninincreased
interstellarlightmaterial
mergingmysteryprimordial
protorawred
rewritingriddlerotating
shiftsignaturesize
smoothlystructuressucking
thirteenuniverseyears

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