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Parameterization of \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 $\gamma ,\, e^{\pm }$ \end{document} , and Neutrino Spectra Produced byp‐pInteraction in Astronomical Environments

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Spectral properties of nonthermal X-ray emission from the shell-type SNR RX J1713.7–3946 as revealed by XMM-Newton

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OBSERVATIONS OF THE YOUNG SUPERNOVA REMNANT RX J1713.7–3946 WITH THEFERMILARGE AREA TELESCOPE

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X-Ray Hotspots in the Northwest Shell of the Supernova Remnant RX J1713.7−3946

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H.E.S.S. observations of RX J1713.7−3946 with improved angular and spectral resolution: Evidence for gamma-ray emission extending beyond the X-ray emitting shell

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Parameterization of the Angular Distribution of Gamma Rays Produced byp‐pInteraction in Astronomical Environments

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Nonthermal emission properties of the northwestern rim of supernova remnant RX J0852.0-4622

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XMM-Newton observations of the supernova remnant RX J1713.7–3946 and its central source

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The INTEGRAL /IBIS Source AX J1838.0-0655: A Soft X-Ray-to-TeV γ-Ray Broadband Emitter

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RXTE,ROSAT, andASCAObservations of G347.3−0.5 (RX J1713.7−3946): Probing Cosmic‐Ray Acceleration by a Galactic Shell‐Type Supernova Remnant

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A High‐Resolution Study of Nonthermal Radio and X‐Ray Emission from Supernova Remnant G347.3−0.5

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The Origin of Nonthermal X‐Ray Filaments and TeV Emission in Young Supernova Remnants

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Expected neutrino signal from supernova remnant RX J1713.7-3946 and flavor oscillations

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Gamma-ray emission from SNR RX J1713.7−3946 and the origin of galactic cosmic rays

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Particle acceleration in cosmic sites

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DERIVATION OF THE ELECTRON DISTRIBUTION IN SUPERNOVA REMNANT RX J1713.7–3946 VIA A SPECTRAL INVERSION METHOD

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On the Gamma-Ray Spectra Radiated by Protons Accelerated in Supernova Remnant Shocks near Molecular Clouds: The case of Supernova Remnant RX J1713.7-3946

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The Slow X-Ray Expansion of the Northwestern Rim of the Supernova Remnant RX J0852.0-4622

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