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 suzakugc.tex AN, 2008, in press
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%astro-ph/0711.2866

\documentclass[mathleft]{an}
\usepackage{graphicx}
\usepackage{times}
\overfullrule5pt
\begin{document}

% The following seven commands are intended for editorial usage and should be ignored by
% the author(s).
\Pagespan{1}{10}% Document's page range.
% If second parameter is left empty, the last page is computed automatically.
\Yearpublication{2006}%
\Yearsubmission{2005}%
\Month{1}%
\Volume{}%
\Issue{1}%
% \DOI{This.is/not.aDOI}%

\title{X-Ray Observations of the Galactic Center with Suzaku}

\author{K. Koyama\thanks{Corresponding author: \email{koyama@cr.scphys.kyoto-u.ac.jp}\newline},
Y. Hyodo,  T. Inui,  M. Nobukawa and  H. Mori}
\titlerunning{Instructions for authors}
\authorrunning{K. Koyama}
\institute{Department of Physics, Graduate School of Science, Kyoto University}

\received{30 May 2005}
\accepted{11 Nov 2005}
\publonline{later}

\keywords{Galactic Center, X-ray, FeK$\alpha$ lines}

\abstract{
We report on the diffuse X-ray emissions from the Galactic center (GCDX) observed with the X-ray Imaging Spectrometer
(XIS) on board the Suzaku satellite. The highly accurate energy calibrations and extremely low background of the XIS
provide many new facts on the GCDX. These are (1) the origin of the 6.7/7.0~keV
lines is
collisional excitation in hot plasma, (2) new SNR and super-bubble candidates are found, (3) most of the 6.4~keV line is
fluorescence by X-rays, and (4) time variability of the 6.4~keV line is found from the Sgr~B2 complex.
}

\maketitle

\end{document}