| dc.contributor.author | Hodne, Espen | |
| dc.date.accessioned | 2019-09-07T23:46:04Z | |
| dc.date.available | 2019-09-07T23:46:04Z | |
| dc.date.issued | 2019 | |
| dc.identifier.citation | Hodne, Espen. Modelling Lyman-α Emission from Star Forming Galaxies at High Redshift Using Cosmological Simulations. Master thesis, University of Oslo, 2019 | |
| dc.identifier.uri | http://hdl.handle.net/10852/69988 | |
| dc.description.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. | eng |
| dc.language.iso | eng | |
| dc.subject | | |
| dc.title | Modelling Lyman-α Emission from Star Forming Galaxies at High Redshift Using Cosmological Simulations | eng |
| dc.type | Master thesis | |
| dc.date.updated | 2019-09-07T23:46:03Z | |
| dc.creator.author | Hodne, Espen | |
| dc.identifier.urn | URN:NBN:no-73120 | |
| dc.type.document | Masteroppgave | |
| dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/69988/1/master_thesis_espen_hodne.pdf | |