
doi: 10.15488/10527
1967 wurde der erste Pulsar als scheinbar pulsierende Radioquelle entdeckt. Seitdem wurden mehr als 2800 weitere Pulsare gefunden, die meisten davon ebenfalls im Radiobereich. Mit dem Start des Fermi Gamma-ray Space Telescope im Jahr 2008 wurden mittlerweile mehr als 250 Gamma-Pulsare entdeckt. Diese Arbeit behandelt die Entwicklung von Suchmethoden, um Gamma-Daten direkt nach Pulsaren in Binärsystemen zu durchsuchen, und präsentiert die Entdeckung und Vermessung von vier solchen Pulsaren.
The first pulsar has been detected in 1967 as a seemingly pulsating radio source. Since then, more than 2800 pulsars have been discovered. Most of them also in radio. With the launch of the Fermi Gamma-ray Space Telescope in 2008, more than 250 gamma-ray pulsars have been detected. This thesis concerns the development of methods to directly search the gamma-ray data for pulsars in binary systems, and presents the discovery and analysis of four such pulsars.
gamma rays, Gamma-Strahlen, Suchmethoden, Neutronensterne, Binär-Pulsare, search methods, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, neutron stars, binary pulsars, Dewey Decimal Classification::500 | Naturwissenschaften, Dewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie, Kartographie
gamma rays, Gamma-Strahlen, Suchmethoden, Neutronensterne, Binär-Pulsare, search methods, Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik, neutron stars, binary pulsars, Dewey Decimal Classification::500 | Naturwissenschaften, Dewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie, Kartographie
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