The complex relations between supernova remnants and neutron stars

Most supernovae (SNe) are expected to produce a neutron star (NS) observable as a radio-loud pulsar. The observations, however, show very few SNRs/NS associations. This review summarizes recent multiwavelength observations carried out to investigate this issue. The work is focused on the current und...

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Detalles Bibliográficos
Publicado:	2002
Materias:	ISM: supernova remnants Stars: neutron stars Stars: pulsars
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v14_n_p43_Dubner http://hdl.handle.net/20.500.12110/paper_14052059_v14_n_p43_Dubner
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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