Is there room for highly magnetized pulsar wind nebulae among those non-detected at TeV?

We make a time-dependent characterization of pulsar wind nebulae (PWNe) surrounding some of the highest spin-down pulsars that have not yet been detected at TeV. Our aim is assessing their possible level of magnetization. We analyse the nebulae driven by J2022+3842 in G76.9+1.0, J0540-6919 in N158A...

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Guardado en:
Detalles Bibliográficos
Publicado: 2014
Materias:
Gamma-rays: ISM
ISM: general
Radiation mechanisms: non-thermal
Stars: neutron
Supernovae:general
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v443_n1_p138_Martin
http://hdl.handle.net/20.500.12110/paper_00358711_v443_n1_p138_Martin
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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