1E161348-5055 Notes et références | Menu de navigationmodifier1E161348-5055voir la liste des auteurs« Young Magnetar Likely the Slowest Pulsar Ever Detected »« Supernova Leaves Behind Mysterious Object »

PulsarConstellation de la Règle


projets correspondantsConsultez la documentation du modèlepulsarrémanent de supernovaRCW 103rayons XEinstein Observatory





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1E161348-5055



Description de cette image, également commentée ci-après

Image de 1E161348-5055 au centre (en bleu) de RCW 103 dans le domaine des rayons X.






Données observationnelles
Constellation
Règle





Caractéristiques

Période Pdisplaystyle P

24 000 s
Âge caractéristique
2 000 années

modifier Consultez la documentation du modèle



1E161348-5055 ou 1E 161348-5055 est un possible pulsar identifié au centre du rémanent de supernova RCW 103. Il s'agit d'une source de rayons X possédant une période d'environ 6,67 heures (24 000 secondes) et âgé d'environ 2 000 ans[1]. Cet objet a été découvert par l'Einstein Observatory[2].



Notes et références |



  • (en) Cet article est partiellement ou en totalité issu de l’article de Wikipédia en anglais intitulé « 1E161348-5055 » (voir la liste des auteurs).


  1. ↑ (en) « Young Magnetar Likely the Slowest Pulsar Ever Detected », sur nasa.gov, 8 septembre 2016.


  2. ↑ (en) « Supernova Leaves Behind Mysterious Object », sur esa.int, 6 juillet 2006.



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