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

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

2006-12-05

arxiv.org/abs/astro-ph/0612129v2

Astronomy and Astrophysics

Astrophysics

Preliminary report, 5 pages, 1 figure; Version 2 has corrected identification of non-X-ray events in figure and text

Scientific paper

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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