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Observations of globular clusters provide a crucial clue to the origin of so-called X-ray binary sources.
They are expected to contribute essentially to study of various astrophysical objects such as AGN, SNe, Gamma-ray bursts (GRBs), X ray flashes (XRFs), galactic binary sources, stars, CVs, X-ray novae, various transient sources, etc.
Let U1 and U2 be two dependent, uniform binary sources.
So why is it, then, that there aren't gravitational waves from binary sources detected in our own galaxy?
Generally speaking, super-Gaussian cases, including binary sources, are extensively used and result in E{G z k )} > E{G} [49] with respect to a proper G function.
This short contribution clarifies very concisely several issues that arise with EXIT charts and nonuniform binary sources (a nonuniform binary source can be the result of a nonbinary source followed by a binary source code).
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symmetric binary source and when decoded would necessarily comply with all considered constraints.
The particular case where the binary source is memoryless with nonuniform symbol probabilities has been studied by Korn et al. [Optimal binary communication with nonequal probabilities.
Mercury-intrusion results furnish auxiliary data that are used for the estimation of a critical percolation diameter and to establish a necessary condition for the binary source images to give accurate predictions of permeability, considering the intrinsic limitations of the reconstruction process.
In both evaluations, the binary source message with p=0.1 is considered.
We consider an i.i.d binary source that generates information blocks U∈{0,1} K.
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