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dark-cosmology.dk /~pela

Dust in Young Galaxies. Ebeltoft, 2008. DARK Cosmology Centre | Niels Bohr Institutet | Københavns Universitet. www.dark-cosmology.dk /~pela. Damped Ly  absorbers, DLA s. Ly  emitters, LAE s. Lyman-break galaxies, LBG s. Sub-mm galaxies, SMG s. Distant red galaxies, DRG s.

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dark-cosmology.dk /~pela

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  1. Dust in Young Galaxies Ebeltoft, 2008 DARK Cosmology Centre| Niels Bohr Institutet | Københavns Universitet www.dark-cosmology.dk/~pela

  2. Damped Ly absorbers, DLAs Ly emitters, LAEs Lyman-break galaxies, LBGs Sub-mm galaxies, SMGs Distant red galaxies, DRGs How to find them?

  3. Selection effects? LBGs/DLAs probe two diff. ends of hi-z LF Viewing angle? Building the bridge Evolutionary sequence? DLA  LAE  LBG  DRG  SMG?

  4. Determinen • ^ • Escape! Monte Carlo • Emit photon •  • Determine t •  • Determine uatom • 

  5. Radiative transfer

  6. Non-isotropic <ESC>

  7. How about dust?

  8. Inhomogeneous medium

  9. Adaptive Mesh Refinement

  10. Adaptive Mesh Refinement

  11. Metals He, C, N, O, Ca, Si, S, Fe at different ionization levels

  12. Metals condense to dust In principle easy: Properties of dust n: , P(,):

  13. Metals condense to dust In principle easy: Properties of dust n: , P(,):

  14. Metals condense to dust In principle easy: Properties of dust n: , P(,):

  15. Metals condense to dust In principle easy: Properties of dust n: , P(,):

  16. Metals condense to dust In principle easy: Properties of dust n: , P(,):

  17. Properties of dust • Laboratory experiments

  18. Properties of dust • Laboratory experiments

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