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
![Open Access](/xmlui/themes/Fakultaeten//images/32px-Open_Access_logo_PLoS_white.svg.png)
dc.contributor.advisor | Kerp, Jürgen | |
dc.contributor.author | Pradas Simón, Juan Enrique | |
dc.date.accessioned | 2020-04-06T21:10:29Z | |
dc.date.available | 2020-04-06T21:10:29Z | |
dc.date.issued | 2004 | |
dc.identifier.uri | https://hdl.handle.net/20.500.11811/2086 | |
dc.description.abstract | 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. | |
dc.language.iso | eng | |
dc.rights | In Copyright | |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | |
dc.subject | X-ray background | |
dc.subject | Galactic Halo | |
dc.subject | 21-cm surveys | |
dc.subject | HVC | |
dc.subject | WHIM | |
dc.subject.ddc | 520 Astronomie, Kartografie | |
dc.title | The hot phase of the ISM | |
dc.title.alternative | Investigation of the soft X-ray background | |
dc.type | Dissertation oder Habilitation | |
dc.publisher.name | Universitäts- und Landesbibliothek Bonn | |
dc.publisher.location | Bonn | |
dc.rights.accessRights | openAccess | |
dc.identifier.urn | https://nbn-resolving.org/urn:nbn:de:hbz:5N-04252 | |
ulbbn.pubtype | Erstveröffentlichung | |
ulbbnediss.affiliation.name | Rheinische Friedrich-Wilhelms-Universität Bonn | |
ulbbnediss.affiliation.location | Bonn | |
ulbbnediss.thesis.level | Dissertation | |
ulbbnediss.dissID | 425 | |
ulbbnediss.date.accepted | 30.09.2004 | |
ulbbnediss.fakultaet | Mathematisch-Naturwissenschaftliche Fakultät | |
dc.contributor.coReferee | Mebold, Ulrich |
Files in this item
This item appears in the following Collection(s)
-
E-Dissertationen (4114)