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Millisecond Dips in Sco X-1 are Likely the Result of High-Energy Particle Events

T. A. Jones·A. M. Levine·E. H. Morgan·S. Rappaport
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Abstract

Chang et al. (2006) reported millisecond duration dips in the X-ray intensity of Sco X-1 and attributed them to occultations of the source by small trans-Neptunian objects (TNOs). We have found evidence that these dips are in fact not astronomical in origin, but rather the result of high-energy charged particle events in the RXTE PCA detectors.

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T. A. Jones, A. M. Levine, E. H. Morgan, S. Rappaport. 2007-02-16. Millisecond Dips in Sco X-1 are Likely the Result of High-Energy Particle Events. https://arxiv.org/abs/astro-ph/0612129

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