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From: "Jim Hinton" <Jim.Hinton@mpi-hd.mpg.de>
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%astro-ph/0607557

\documentstyle{article} (your LaTex file goes into the body of the email)
\begin{document}

  \title{Inverse Compton Scenarios for the TeV Gamma-Ray Emission
    of the Galactic Centre
  }

\author{J. A. Hinton}

\affil{Max-Planck-Institut f\"ur Kernphysik, P.O. Box 103980, D 69029
Heidelberg, Germany}
\affil{Landessternwarte, Universit\"at Heidelberg, K\"onigstuhl, D 69117
Heidelberg, Germany}

\author{F. A. Aharonian}

\affil{Max-Planck-Institut f\"ur Kernphysik, P.O. Box 103980, D 69029
Heidelberg, Germany}

\begin{abstract}

The intense Compton cooling of ultra-relativistic electrons in the
Klein-Nishina regime in radiation dominated
environments, such as that found in the Galactic Centre, may result in
radically different electron spectra than those produced by
Synchrotron cooling.  We explore these effects and their impact on the
X-ray and $\gamma$-ray spectra produced in electron accelerators in
this region in comparison to elsewhere in our galaxy. We discuss the
broad-band emission expected from the newly discovered pulsar wind
nebula G\,359.95$-$0.04 and the possible relationship of this X-ray
source to the central TeV $\gamma$-ray source HESS\,J1745$-$290.
Finally we discuss the possible relationship of the Galactic Centre
INTEGRAL source IGR\,J1745.6$-$2901 to the TeV emission.

\end{abstract}

\end{document}