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Constraining the Coronal Heights and Readjustment Velocities Based on the Detection of a Few Hundred Seconds Delays in the Z Source GX 17+2

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ALMA observations of 4U 1728−34 and 4U 1820−30: first detection of neutron star X-ray binaries at 300 GHz

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Suzaku studies of luminosity-dependent changes in the low-mass X-ray binary Aquila X-1

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The type I X-ray bursts of 4U 1735–44

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Spectral states evolution of 4U 1728-34 observed by INTEGRAL and RXTE: non-thermal component detection

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The Hard X‐Ray Tails in Neutron Star Low‐Mass X‐Ray Binaries:BeppoSAXObservations and Possible Theoretical Explanation of the Case of GX 17 \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $+$ \end{document} 2

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