Antiglitch Inconsistent With Magnetar Model of AXP
Fuente:
arXiv
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| Autore principale: | |
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| Natura: | Preprint |
| Pubblicazione: |
2013
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| _version_ | 1866909189732827136 |
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| author | Katz, J. I. |
| author_facet | Katz, J. I. |
| 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_1307_0586 |
| institution | arXiv |
| publishDate | 2013 |
| record_format | arxiv |
| spellingShingle | Antiglitch Inconsistent With Magnetar Model of AXP Katz, J. I. High Energy Astrophysical Phenomena 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. |
| title | Antiglitch Inconsistent With Magnetar Model of AXP |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/1307.0586 |