arXiv · astro-ph/9712254
Recent Results on the Anomalous X-ray Pulsars
Abstract
The ''Anomalous X-ray Pulsars'' (AXPs) are a small group of X-ray pulsars characterized by periods in the 5-10 s range and by the absence of massive companion stars. There are now 7 possible members of this class of objects. We review recent observational results on their X-ray spectra, spin period evolution, and searches for orbital motion and discuss the implications for possible models.
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S. Mereghetti, L. Stella, G. L. Israel. 1997-12-18. Recent Results on the Anomalous X-ray Pulsars. https://doi.org/10.1016/s0920-5632(98)00220-5
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