The hot phase of the ISMInvestigation of the soft X-ray background
The hot phase of the ISM
Investigation of the soft X-ray background
Dokument öffnen (5.9MB)Art der Hochschulschrift
DissertationPrüfungsdatum
30.09.2004Datum der Veröffentlichung
2004Erstgutachter
Kerp, JürgenZweitgutachter
Mebold, UlrichMetadaten
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Inhalt
In this thesis I present a quantitative solution of the soft X-ray radiation transfer through the Galactic interstellar medium. I focus on the Galactic Halo emission because its intensity distribution is thought to trace the shape of the Milky Way's Dark Matter gravitational potential. The best fit model for the soft X-ray background allows to identify areas in the sky which deviate significantly from the this solution. These areas are associated with high-velocity cloud (HVC) complexes or possibly with the warm/hot intergalactic medium. Moreover, it is feasible to estimate lower distance limits to the HVC complexes.
Schlagwörter
X-ray background, Galactic Halo, 21-cm surveys, HVC, WHIM
Klassifikation (DDC)
520 Astronomie, KartografiePradas Simón, Juan Enrique: The hot phase of the ISM : Investigation of the soft X-ray background. - Bonn, 2004. - Dissertation, Rheinische Friedrich-Wilhelms-Universität Bonn.
Online-Ausgabe in bonndoc: https://nbn-resolving.org/urn:nbn:de:hbz:5N-04252
Online-Ausgabe in bonndoc: https://nbn-resolving.org/urn:nbn:de:hbz:5N-04252
@phdthesis{handle:20.500.11811/2086,
urn: https://nbn-resolving.org/urn:nbn:de:hbz:5N-04252,
author = {{Juan Enrique Pradas Simón}},
title = {The hot phase of the ISM : Investigation of the soft X-ray background},
school = {Rheinische Friedrich-Wilhelms-Universität Bonn},
year = 2004,
note = {In this thesis I present a quantitative solution of the soft X-ray radiation transfer through the Galactic interstellar medium. I focus on the Galactic Halo emission because its intensity distribution is thought to trace the shape of the Milky Way's Dark Matter gravitational potential. The best fit model for the soft X-ray background allows to identify areas in the sky which deviate significantly from the this solution. These areas are associated with high-velocity cloud (HVC) complexes or possibly with the warm/hot intergalactic medium. Moreover, it is feasible to estimate lower distance limits to the HVC complexes.},
url = {https://hdl.handle.net/20.500.11811/2086}
}
urn: https://nbn-resolving.org/urn:nbn:de:hbz:5N-04252,
author = {{Juan Enrique Pradas Simón}},
title = {The hot phase of the ISM : Investigation of the soft X-ray background},
school = {Rheinische Friedrich-Wilhelms-Universität Bonn},
year = 2004,
note = {In this thesis I present a quantitative solution of the soft X-ray radiation transfer through the Galactic interstellar medium. I focus on the Galactic Halo emission because its intensity distribution is thought to trace the shape of the Milky Way's Dark Matter gravitational potential. The best fit model for the soft X-ray background allows to identify areas in the sky which deviate significantly from the this solution. These areas are associated with high-velocity cloud (HVC) complexes or possibly with the warm/hot intergalactic medium. Moreover, it is feasible to estimate lower distance limits to the HVC complexes.},
url = {https://hdl.handle.net/20.500.11811/2086}
}
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