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Det matematisk-naturvitenskapelige fakultet
Institutt for teoretisk astrofysikk
Institutt for teoretisk astrofysikk
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Det matematisk-naturvitenskapelige fakultet
Institutt for teoretisk astrofysikk
Institutt for teoretisk astrofysikk
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Modelling Lyman-α Emission from Star Forming Galaxies at High Redshift Using Cosmological Simulations
Hodne, Espen
Master thesis
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master_thesis_espen_hodne.pdf (3.196Mb)
Year
2019
Permanent link
http://urn.nb.no/
URN:NBN:no-73120
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Institutt for teoretisk astrofysikk
[1306]
Abstract
I calculate Lyman-α luminosity and surface brightness; and find that the values are much higher than typical for this kind of galaxy. I find this is due to very high star formation rate; which makes the galaxy superluminous.
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