Pulse Emission Mechanisms in Pulsars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 23 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Giant Pulses from PSR B1937+21 with Widths ≤15 Nanoseconds and \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 $T_{b}\geq 5\times 10^{39}$ \end{document} K, the Highest Brightness Temperature Observed in the Universe;The Astrophysical Journal;2004-11-20
2. Polarization Properties of Nine Southern Radio Pulsars;The Astronomical Journal;2001-10
3. Birefringence as a Mechanism for the Broadening and Depolarization of Pulsar Average Profiles;The Astrophysical Journal;1997-02
4. Relativistic beaming of the pulsar emission;Monthly Notices of the Royal Astronomical Society;1982-03
5. 100 nanosecond time resolution observations of PSR 1133 + 16;The Astrophysical Journal;1982-03
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