Fermi bubbles: high-latitude X-ray supersonic shell
Author:
Affiliation:
1. Physics Department, Ben-Gurion University of the Negev, POB 653, Be’er Sheva 84105, Israel
2. Department of Physics, NRCN, POB 9001, Be’er Sheva 84190, Israel
Funder
German-Israeli Foundation for Scientific Research and Development
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/480/1/223/25230261/sty1533.pdf
Reference55 articles.
1. THE SPECTRUM AND MORPHOLOGY OF THEFERMIBUBBLES
2. ChandraX‐Ray Spectroscopic Imaging of Sagittarius A* and the Central Parsec of the Galaxy
3. Origins of the \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 $\frac{1}{4}$ \end{document} keV Soft X‐Ray Background
4. Galaxy formation theory
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