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Linking Jet Emission, X‐Ray States, and Hard X‐Ray Tails in the Neutron Star X‐Ray Binary 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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A very rare triple-peaked type-I X-ray burst in the low-mass X-ray binary 4U 1636−53

Guobao Zhang, Mariano Méndez, Diego Altamirano, Tomaso M. Belloni and Jeroen Homan
Monthly Notices of the Royal Astronomical Society 398 (1) 368 (2009)
DOI: 10.1111/j.1365-2966.2009.15148.x
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