Et fordrag om stjerner og m

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Dust in Young Galaxies
Peter Laursen Supervisor Anja C. Andersen
www.dark-cosmology.dk DARK
Cosmology Centre Niels Bohr Institutet
Københavns Universitet
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The code
Radiative transfer
Monte Carlo
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Results
Surface brightness maps
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Results
Surface brightness maps Surface
brightness profiles
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Results
Surface brightness maps Surface
brightness profiles Spectra
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Dust in Young Galaxies
Star formation Dust formation Dust
destruction Radiative transfer
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Dust in Young Galaxies
Dust Extinction in Starburst Galaxies at z 3
6 Dust Creation in Supernova Explosions Lyman a
Galaxies at z 8.8
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Dust Extinction in Starburst Galaxies at
z 3 - 6
Lyman-Break Galaxies SFR 10 1000 M
yr-1 Correcting for dust with Calzetti ext.
curve SFR increases a factor of 2 5
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Dust Extinction in Starburst Galaxies at
z 3 - 6
Advance Monte Carlo code Predict effect of dust
as function of tsf, Z and z Very young
starbursts No AGBs, intense UV field Analyze and
model SED of LBGs from GOODS z 2 6
X-rays to mid-IR and Ultra-VISTA (COSMOS
field)
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Dust Creation in Supernova
Explosions
No AGB stars ? SNe? Grain formation and growth
in SN remnants
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Lyman a Galaxies at z 8.8
no sky-lines in the near-IR e.g., l 1.2
mm Simulate morphology and SB of statistical
sample Compare with VISTA observations