Time-dependent modeling of TeV-detected, young pulsar wind nebulae

The increasing sensitivity of instruments at X-ray and TeV energies has revealed a large number of nebulae associated with bright pulsars. Despite this large data set, the observed pulsar wind nebulae (PWNe) do not show a uniform behavior and the main parameters driving features like luminosity, mag...

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Detalles Bibliográficos
Autores principales:	Torres, D.F., Cillis, A., Martín, J., de Oña Wilhelmi, E.
Formato:	JOUR
Materias:	Pulsars: general Radiation mechanisms: non-thermal
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_22144048_v1-2_n_p31_Torres
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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