Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies
Lasting anywhere from a few milliseconds to several minutes, GRBs shine hundreds of times brighter than a typical supernova, making them briefly the brightest source of cosmic gamma-ray photons in the observable Universe. This thesis focuses on 3 different aspects of GRBs: (1) The radiative mechanis...
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ftdatacite:10.48550/arxiv.1512.03205 2023-05-15T16:48:58+02:00 Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies Friis, Mette 2015 https://dx.doi.org/10.48550/arxiv.1512.03205 https://arxiv.org/abs/1512.03205 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Preprint Article article CreativeWork 2015 ftdatacite https://doi.org/10.48550/arxiv.1512.03205 2022-04-01T11:34:18Z Lasting anywhere from a few milliseconds to several minutes, GRBs shine hundreds of times brighter than a typical supernova, making them briefly the brightest source of cosmic gamma-ray photons in the observable Universe. This thesis focuses on 3 different aspects of GRBs: (1) The radiative mechanism of GRBs and their afterglows, i.e. the occurrence of thermal emission and the physical parameters we can determine through this emission. (2) Their host galaxies, using results from observations of GRB 121024A as a case study. (3) How they can be used to answer some of the larger astrophysical questions, more specifically in this case, to study interstellar dust and grey extinction. : PhD dissertation, University of Iceland, Reykjav\'ik, October 2015 Report Iceland DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
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High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Friis, Mette Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies |
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High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
Lasting anywhere from a few milliseconds to several minutes, GRBs shine hundreds of times brighter than a typical supernova, making them briefly the brightest source of cosmic gamma-ray photons in the observable Universe. This thesis focuses on 3 different aspects of GRBs: (1) The radiative mechanism of GRBs and their afterglows, i.e. the occurrence of thermal emission and the physical parameters we can determine through this emission. (2) Their host galaxies, using results from observations of GRB 121024A as a case study. (3) How they can be used to answer some of the larger astrophysical questions, more specifically in this case, to study interstellar dust and grey extinction. : PhD dissertation, University of Iceland, Reykjav\'ik, October 2015 |
format |
Report |
author |
Friis, Mette |
author_facet |
Friis, Mette |
author_sort |
Friis, Mette |
title |
Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies |
title_short |
Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies |
title_full |
Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies |
title_fullStr |
Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies |
title_full_unstemmed |
Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies |
title_sort |
exploring gamma-ray bursts, their immediate environment and host galaxies |
publisher |
arXiv |
publishDate |
2015 |
url |
https://dx.doi.org/10.48550/arxiv.1512.03205 https://arxiv.org/abs/1512.03205 |
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Iceland |
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Iceland |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1512.03205 |
_version_ |
1766039042438201344 |