------------------------------------------------------------------------ clenet.tex A&A, 2005, 439, L9 Date: Mon, 12 Sep 2005 15:33:13 +0200 X-Mailer: Apple Mail (2.622) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mesiob.obspm.fr [145.238.2.2]); Mon, 12 Sep 2005 15:32:10 +0200 (CEST) X-Virus-Scanned: ClamAV version 0.86.2, clamav-milter version 0.86 on mesiob.obspm.fr X-Virus-Status: Clean X-MailScanner-Information: Please contact postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=0, required 5, autolearn=disabled) X-MailScanner-From: yann.clenet@obspm.fr %astro-ph/0507088 \documentclass[twocolumn]{aa} \usepackage{graphicx,natbib,textcomp} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \usepackage{txfonts} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% % \begin{document} % \title{A dual emission mechanism in \object{Sgr A*/L$^\prime$} ?\thanks{Based on observations collected at the ESO VLT Yepun telescope, proposal 073.B-0665}} \author{Y. Cl\'enet\inst{1} \and D. Rouan\inst{1} \and D. Gratadour\inst{1} \and O. Marco\inst{2} \and P. L\'ena\inst{1} \and N. Ageorges\inst{2} \and E. Gendron\inst{1} } \offprints{Y. Cl\'enet} \institute{ Observatoire de Paris, LESIA, 5 place Jules Janssen, F-92195 Meudon Cedex, France\\ \email{firstname.lastname@obspm.fr} \and European Southern Observatory (ESO), Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19, Chile\\ \email{nageorges@eso.org, omarco@eso.org} } \date{Received 28 April 2005 / Accepted 26 June 2005} \abstract{We have collected in 2004 adaptive optics corrected L$^\prime$ images of the Galactic Center region with NAOS-CONICA at VLT. A strong variability was observed as well as a correlation between the photocenter positions and fluxes of the L$^\prime$-band counterpart of \object{Sgr~A*}. It is interpreted as the combined emission of a point-like flaring source at the position of \object{Sgr~A*/IR} itself and an extended dust structure, 75 mas south west of \object{Sgr~A*/IR}, which we name \object{Sgr~A*-f}. We examine the different possible mechanisms to explain this dual \object{Sgr~A*} L$^\prime$ emission and conclude it is likely a flaring emission associated to energetic events in the close environment of the black hole plus a quiescent emission resulting from the collision of \object{Sgr~A*-f} by a jet from \object{Sgr~A*}. \keywords{Galaxy: center -- Infrared: stars -- Instrumentation : adaptive optics} } \maketitle \end{document}