Modeling the emission of the Galactic very high energy [gamma]-ray sources G1.9+0.3, G330.2+1.0, HESS J1303-631 and PSR B1259-63/LS 2883 observed with H.E.S.S.
dc.contributor.author | Sushch, Iurii | |
dc.date.accessioned | 2017-06-18T12:04:26Z | |
dc.date.available | 2017-06-18T12:04:26Z | |
dc.date.created | 2013-02-26 | |
dc.date.issued | 2013-01-29 | |
dc.identifier.uri | http://edoc.hu-berlin.de/18452/17326 | |
dc.description.abstract | Abbildende Cherenkov-Teleskope haben in den letzten Jahren eine groẞe Anzahl neuer Gammastrahlungsquellen im Bereich sehr hoher Energien (VHE, very high energy, E>100 GeV) entdeckt. Diese Studie behandelt Vertreter von drei unterschiedlichen Klassen von galaktischen Gammastrahlungsquellen: die Supernova-Überreste G1.9+0.3 und G330.2+1.0, den Pulsarwind-Nebel HESS J1303-631 und das Binärsystem PSR B1259-63/LS 2883. Für alle Objekte werden die Analyse der H.E.S.S.-Daten und die Modellierung der Emission unter Einbeziehung von Daten aus anderen Wellenlängenbereichen dargestellt. | ger |
dc.description.abstract | Recently, imaging atmospheric Cherenkov telescopes have discovered numerous new sources representing various source classes in the very high energy (VHE; E>100 GeV) sky. This work presents studies of representatives of three types of Galactic VHE emitters: the Supernova remnants G1.9+0.3 and G330.2+1.0, the pulsar wind nebula HESS J1303-631 and the binary system PSR B1259-63/LS 2883. The analysis of the H.E.S.S. data and the broadband emission modeling are presented. | eng |
dc.language.iso | eng | |
dc.publisher | Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I | |
dc.rights | Namensnennung - Keine kommerzielle Nutzung - Keine Bearbeitung | |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/de/ | |
dc.subject | H.E.S.S. | ger |
dc.subject | Gammaastronomie | ger |
dc.subject | Supernova-Überrest | ger |
dc.subject | Pulsarwind-Nebel | ger |
dc.subject | Binärsystem | ger |
dc.subject | H.E.S.S. | eng |
dc.subject | gamma-ray astronomy | eng |
dc.subject | supernova remnant | eng |
dc.subject | pulsar wind nebula | eng |
dc.subject | binary system | eng |
dc.subject.ddc | 530 Physik | |
dc.title | Modeling the emission of the Galactic very high energy [gamma]-ray sources G1.9+0.3, G330.2+1.0, HESS J1303-631 and PSR B1259-63/LS 2883 observed with H.E.S.S. | |
dc.type | doctoralThesis | |
dc.identifier.urn | urn:nbn:de:kobv:11-100207464 | |
dc.identifier.doi | http://dx.doi.org/10.18452/16674 | |
dc.identifier.alephid | BV040777228 | |
dc.date.accepted | 2012-10-19 | |
dc.contributor.referee | Lohse, Thomas | |
dc.contributor.referee | Maier, Gernot | |
dc.contributor.referee | Aharonian, Felix | |
dc.subject.dnb | 29 Physik, Astronomie | |
dc.subject.rvk | UN 7000 | |
dc.subject.rvk | UO 9500 | |
local.edoc.pages | 155 | |
local.edoc.type-name | Dissertation | |
bua.department | Mathematisch-Naturwissenschaftliche Fakultät I |