The complex relations between supernova remnants and neutron stars

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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
Autor principal: Dubner, G.
Formato: CONF
Materias:
ISM: supernova remnants
Stars: neutron stars
Stars: pulsars
Acceso en línea: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 todo:paper_14052059_v14_n_p43_Dubner
record_format dspace
spelling todo:paper_14052059_v14_n_p43_Dubner2023-10-03T16:12:52Z The complex relations between supernova remnants and neutron stars Dubner, G. 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). CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar 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
Dubner, G.
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).
format CONF
author Dubner, G.
author_facet Dubner, G.
author_sort Dubner, G.
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
url http://hdl.handle.net/20.500.12110/paper_14052059_v14_n_p43_Dubner
work_keys_str_mv AT dubnerg thecomplexrelationsbetweensupernovaremnantsandneutronstars
AT dubnerg complexrelationsbetweensupernovaremnantsandneutronstars
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