Abstract
Here we discuss experimental studies over long observation intervals (13 years) of the statistical stability of X-ray radiation from three astrophysical objects. It is found that all the studied radiation intensities are statistically unstable. The most stable oscillations are from the pulsar PSRJ 1012 + 5307. It is found that, over the whole observation interval, its oscillations are statistically stable with respect to the average, but unstable with respect to the standard deviation.
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Gorban, I.I. (2017). Experimental Studies of the Statistical Stability of Radiation from Astrophysical Objects. In: The Statistical Stability Phenomenon. Mathematical Engineering. Springer, Cham. https://doi.org/10.1007/978-3-319-43585-5_7
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DOI: https://doi.org/10.1007/978-3-319-43585-5_7
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