AXPs and SGRs in the outer gap model: confronting Fermi observations
arXiv:1101.2289 · doi:10.1088/0004-637X/738/1/31
Abstract
Anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are magnetar candidates, i.e., neutron stars powered by strong magnetic field. If they are indeed magnetars, they will emit high-energy gamma-rays which are detectable by Fermi-LAT according to the outer gap model. However, no significant detection is reported in recent Fermi-LAT observations of all known AXPs and SGRs. Considering the discrepancy between theory and observations, we calculate the theoretical spectra for all AXPs and SGRs with sufficient observational parameters. Our results show that most AXPs and SGRs are high-energy gamma-ray emitters if they are really magnetars. The four AXPs 1E 1547.0-5408, XTE J1810-197, 1E 1048.1-5937, and 4U 0142+61 should have been detected by Fermi-LAT. Then there is conflict between out gap model in the case of magnetars and Fermi observations. Possible explanations in the magnetar model are discussed. On the other hand, if AXPs and SGRs are fallback disk systems, i.e., accretion-powered for the persistent emissions, most of them are not high-energy gamma-ray emitters. Future deep Fermi-LAT observations of AXPs and SGRs will help us make clear whether they are magnetars or fallback disk systems.
15 pages, 3 figures, 1 table, accepted for publication in The Astrophysical Journal
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Cited by in corpus (15)
- Wind braking of magnetars
- SGR 0418+5729 - How does a Young Neutron Star Spin Down to a 9 s Period with a Dipole Field less than 10^13 G?
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- GeV detection of HESS J0632+057
- Pulsar braking: magnetodipole vs. wind
- Magnetars and White Dwarf Pulsars
- Soft gamma-ray repeaters and anomalous X-ray pulsars as highly magnetized white dwarfs
- Magnetars: fact or fiction?
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