The Island state of the Atoll Source 4U 1820--30
arXiv:astro-ph/0507097 · doi:10.1086/447761
Abstract
We study the rapid X-ray time variability in all public data available from the \textit{Rossi X-ray Timing Explorer's} Proportional Counter Array on the atoll source 4U 1820--30 in the low-luminosity island state. A total of ks of data were used. We compare the frequencies of the variability components of 4U 1820--30 with those in other atolls sources. These frequencies were previously found to follow a universal scheme of correlations. We find that 4U 1820--30 shows correlations that are shifted by factors of and with respect to those in other atoll sources. These shifts are similar to, but smaller than the shift factor previously reported for some accreting millisecond pulsars. Therefore, 4U 1820--30 is the first atoll source which shows no significant pulsations but has a significant shift in the frequency correlations compared with other 3 non-pulsating atoll sources.
arXiv comment21 pages, 8 Figures, submitted to ApJ
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