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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Guardado en:
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
id paper:paper_14052059_v14_n_p43_Dubner
record_format dspace
spelling paper:paper_14052059_v14_n_p43_Dubner2023-06-08T16:13:16Z The complex relations between supernova remnants and neutron stars ISM: supernova remnants Stars: neutron stars Stars: pulsars 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 understanding of pulsar wind nebulae (PWN), and the different ways in which a NS can manifest, like anomalous X-ray pulsars (AXPs), radio-quiet neutron stars (RQNS) and soft gamma-ray repeaters (SGRs). 2002 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
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic ISM: supernova remnants
Stars: neutron stars
Stars: pulsars
spellingShingle ISM: supernova remnants
Stars: neutron stars
Stars: pulsars
The complex relations between supernova remnants and neutron stars
topic_facet ISM: supernova remnants
Stars: neutron stars
Stars: pulsars
description 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 understanding of pulsar wind nebulae (PWN), and the different ways in which a NS can manifest, like anomalous X-ray pulsars (AXPs), radio-quiet neutron stars (RQNS) and soft gamma-ray repeaters (SGRs).
title The complex relations between supernova remnants and neutron stars
title_short The complex relations between supernova remnants and neutron stars
title_full The complex relations between supernova remnants and neutron stars
title_fullStr The complex relations between supernova remnants and neutron stars
title_full_unstemmed The complex relations between supernova remnants and neutron stars
title_sort complex relations between supernova remnants and neutron stars
publishDate 2002
url 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
_version_ 1768542001283727360

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