------------------------------------------------------------------------
From: Michael.Nord@nrl.navy.mil
To: gcnews@zia.aoc.nrao.edu
Subject: submit sgrastar330.tex ApJL, Accepted


%astro-ph/0312219

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\begin{document}



%
% 
\newcommand{\mjybm}{\mbox{mJy~beam${}^{-1}$}}
\newcommand{\sgrastar}{\protect\objectname[]{Sgr~A$^{*}$}}
\newcommand{\htwo}{\ion{H}{2}}

\shorttitle{\sgrastar\ at~330~MHz}
\shortauthors{Nord et al.}


\title{Detection of Sagittarius~A$^*$ at~330~MHz with the Very Large 
Array}


\author{Michael E.~Nord, T.~Joseph~W.~Lazio, Namir~E.~Kassim}
\affil{Naval Research Laboratory, Code~7213, Washington, DC  20375-5351}
\email{Michael.Nord@nrl.navy.mil}
\email{Joseph.Lazio@nrl.navy.mil}
\email{Namir.Kassim@nrl.navy.mil}
\altaffiltext{1}{Department of Physics and Astronomy, University of New 
Mexico}

\author{W.~M.~Goss}
\affil{National Radio Astronomy Observatory, P.O.~Box~0, Socorro, NM 
87801}
\email{mgoss@nrao.edu}

\and
\author{N.~Duric}
\affil{Department of Physics and Astronomy, University of New Mexico, 800 
Yale 
Boulevard NE, Albuquerque, NM  87131}
\email{duric@tesla.phys.unm.edu}

\begin{abstract}

We report the detection of Sagittarius~A$^*$, the radio source associated 
with our 
Galaxy's central massive black hole, at 330 MHz with the Very Large Array.  
Implications for the 
spectrum and emission processes of Sagittarius~A$^*$ are discussed and 
several hypothetical geometries of the central region are considered.


\end{abstract}

\keywords{Galaxy: center --- Galaxy: nucleus}