A new study towards PSR J1826-1334 and PSR J1826-1256 in the region of HESS J1825-137 and HESS J1826-130

Aims. The goal of this paper is to detect synchrotron emission from the relic electrons of the crushed pulsar wind nebula (PWN) HESS J1825-137 and to investigate the origin of the γ-ray emission from HESS J1826-130. Methods. The study of HESS J1825-137 was carried out on the basis of new radio obser...

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Detalles Bibliográficos
Autores principales: Duvidovich, L., Giacani, E., Castelletti, G., Petriella, A., Supán, L.
Formato: JOUR
Materias:
Gamma rays: ISM
ISM: individual objects: HESS J1825-137
ISM: individual objects: HESS J1826-130
Radio continuum: ISM
X-rays: ISM
Energy dispersive X ray analysis
Pulsars
X ray diffraction analysis
X rays
Gamma rays: isms
Gamma-ray emission
ISM: individual objects
Pulsar wind nebulae
Synchrotron emission
Very high energies
X rays: ISM
Gamma rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v623_n_p_Duvidovich
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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