The complex relations between Supernova Remnants and Neutron Stars
Most supernovae (SNe) are expected to produce a neutron star (NS) observ-able as a radio-loud pulsar. The observations, however, show very few SNRs/NSassociations. This review summarizes recent multiwavelength observations carriedout to investigate this issue. The work is focused on the current unde...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Hovedforfatter: | |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2002
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| Online adgang: | https://www.redalyc.org/articulo.oa?id=57101426 |
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