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Some results of high-speed two-channel photometry of Wolf-Rayet stars with suspected compact companions
Published online by Cambridge University Press: 07 August 2017
Abstract
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Strong transient chaotic high-frequency activity has been detected in WR148 on a time scale of a few minutes. The main property is the variability of the fluctuation power, not the light-curve. The same is true for WR136 but with a more permanent pattern. The power of fluctuations is of order of thousandth relative to the steady intensity. The maximum fluctuation power lies in the frequency band of 25–50 Hz.
- Type
- Session VIII - Hydrodynamics and high-energy physics of winds accreting on neutrons stars and black holes
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- Copyright © Kluwer 1995
References
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