(NAS Colloquium) The Age of the Universe, Dark Matter, and Structure Formation (1998) / Chapter Skim
Currently Skimming:
The universe at z > 5: When and how did the 'dark age' end?
The universe at z > 5: When and how did the 'dark age' end?
Pages 47-52
The Chapter Skim interface presents what we've algorithmically identified as the most significant single chunk of text within every page in the chapter.
Select key terms on the right to highlight them within pages of the chapter.
From page 47... ...
.. 1rre~ular~le~ on scales elf 10 Observed cosmic structure and on larger scales that are -tin in 1be ~:i:ne~r regime.
|
From page 48... ...
Because of ibis steep 1cmper~turc dependence. Gas ~ this regime contracts almost isoth~rm~l6~ so that as jeans mass decreases as 1b~ drowsily rises.
|
From page 49... ...
lo UV-1~h~tt r~bc~ted old ~pl~o~t~sT~so~iz~/d tube IBM before Cameron wars abet Armed ~ dark maker dues Huh 101~1 mass greater than T03 solar muses Aid internal velocity dispersion greater Oh about jig k~m/sc~c. What is tile chance fig ~ Abut ~ ~ ?
|
From page 50... ...
14 and I Some moderately masses galaxies ara in ~ case Expected to gram before rcio~niz~t~io~, because tile power sputum at small scales in cold dark matter models flattens to ~ Hope of about ~ ~ -2.7 (so the a~lLude of fluctu~t10~s decreases vary J~6 fish scaIc)
|
From page 51... ...
. Was, coven tbou~b tb~e- Oman ~ emission line mig~bt -not bo as <~d ~ Aural Euro ~8 the Peterson trout ~ tc~b~iquetoseatch ~Ugb,~dshi~ ~al~ie,i~ presenceor absence sho~1d~be ~im~pOrl~il~t d~i~ynoEsl!
|
From page 52... ...
~ |
Key Terms
This material may be derived from roughly machine-read images, and so is provided only to facilitate research.
More
information on Chapter Skim is available.