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| Main Author: | |
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| Format: | Preprint |
| Published: |
2013
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/1307.0586 |
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Table of Contents:
- The recently observed antiglitch of AXP 1E 2259+586 is inconsistent with magnetar models, but may be explained as the consequence of sudden accretion of retrograde matter or "propeller" interaction with surrounding matter. AXP/SGR are explained as single neutron stars accompanied by fallback matter from their natal supernovae. Their phenomenology may be partly accretional and partly the result of dissipation of magnetic energy.