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%  Este ejemplo define el formato para el envío de contribuciones a las      %
%  Reuniones Anuales de la Asociación Argentina de Astronomía, a partir      %
%  de 2014. Los resúmenes enviados serán publicados sin modificaciones       %
%  en el Cuaderno de Resúmenes de la Asociación (CRAAA).                     %
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%  ************************** IMPORTANT NOTICE **************************    %
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%  This template defines the format for the submission of contributions      %
%  to the Annual Meetings of the Argentinian Astronomical Association,       %
%  since 2014. The submitted abstracts will be published without changes     %
%  in the Abstract Book of the Association (CRAAA).                          %
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%  The comments in this file give instructions about its mandatory format.   %
%  Please read them.                                                         %
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%  The use of \newcommand and author's definitions are forbidden.            %
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\documentclass[craaa]{aaa2014}

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\usepackage[spanish,activeacute,english]{babel}
\usepackage[utf8]{inputenc}
\usepackage{verbatim}
\usepackage{amsmath}
\usepackage{amsfonts}
\usepackage{amssymb}

\begin{document}

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\journalvol{57}
\journalyear{2014}
\journaleditors{A.C. Rovero, C. Beaugé, L.J. Pellizza, M. Lares}

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%  0: Castellano / Spanish                                                   %
%  1: Inglés / English                                                       %
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\contriblanguage{0}

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%  Seleccione el tipo de contribución solicitada:                            %
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%  Select the requested contribution type:                                   %
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%  1: Presentación mural / Poster                                            %
%  2: Presentación oral / Oral contribution                                  %
%  3: Informe invitado / Invited report                                      %
%  4: Mesa redonda / Round table                                             %
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\contribtype{2}

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%  Seleccione el área temática de su contribución:                           %
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%  Select the thematic area of your contribution:                            %
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%  11 [AEC]: Astrofísica Extragaláctica y Cosmología /                       %
%           Extragalactic Astrophysics and Cosmology                         %
%  12 [EG]: Estructura Galáctica / Galactic Structure                        %
%  13 [AE]: Astrofísica Estelar / Stellar Astrophysics                       %
%  14 [SE]: Sistemas Estelares / Stellar Systems                             %
%  15 [ICSA]: Instrumentación y Caracterización de Sitios Astronómicos /     %
%            Instrumentation and Astronomical Site Characterization          %
%  16 [MI]: Medio Interestelar / Interstellar Medium                         %
%  17 [OCPAE]: Objetos Compactos y Procesos de Altas Energías /              %
%             Compact Objetcs and High-Energy Processes                      %
%  18 [SH]: Sol y Heliosfera / Sun and Heliosphere                           %
%  19 [SSE]: Sistemas Solar y Extrasolares / Solar and Extrasolar Systems    %
%  21 [HEDA]: Historia, Enseñanza y Divulgación de la Astronomía /           %
%             History, Teaching and Spreading of Astronomy                   %
%  22 [O]: Otros / Other Topics                                              %
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\thematicarea{11}

\title{Morfología de galaxias enanas en simulaciones num\'ericas}

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\author{Sales L.V.\inst{1}}

\institute{Harvard University}

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\abstract{La morfología de las galaxias enanas es claramente diferente a la de galaxias mas masivas como la
Via L\'actea o Andr\'omeda. En esta contribuci\'on voy a presentar resultados sobre posibles causas de estas diferencias
estructurales; con especial atenci\'on a: i) el efecto de la eficiencia bari\'onica (fracci\'on de gas y estrellas
comparada con la masa virial) en galaxias de diferente masa, ii) interacci\'on con subhalos dentro de CDM y 
iii) efectos de "feedback" estelar en los discos gaseosos. Los resultados estar\'an basados en simulaciones 
hidrodin\'amicas que son corroborados por observaciones de galaxies enanas en el vol\'umen local.}

%\abstractLa {morfología de las galaxias enanas es claramente diferente a la de galaxias mas masivas como la
%Via L\'actea o Andr\'omeda. En esta contribuci\'on voy a presentar resultados sobre posibles causas de estas diferencias
%estructurales; con especial atenci\'on a: i) el efecto de la eficiencia bari\'onica (fracci\'on de gas y estrellas
%comparada con la masa virial) en galaxias de diferente masa, ii) interacci\'on con subhalos dentro de CDM y 
%iii) efectos de "feedback" estelar en los discos gaseosos. Los resultados estar\'an basados en simulaciones 
%hidrodin\'amicas que son corroborados por observaciones de galaxies enanas en el vol\'umen local.}


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%  Seleccione las palabras clave que describen su contribución. Las mismas   %
%  son obligatorias, y deben tomarse de la lista de la American Astronomical %
%  Society (AAS), que se encuentra en la página web indicada abajo.          %
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%  Select the keywords that describe your contribution. They are mandatory,  %
%  and must be taken from the list of the American Astronomical Society      %
%  (AAS), which is available at the webpage quoted below.                    %
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\keywords{galaxies: dwarf --- galaxies: formation --- galaxies: structure}

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% Por favor provea una dirección de e-mail de contacto para los lectores.    %
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% Please provide a contact e-mail address for readers.                       %
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\mail{lsales@cfa.harvard.edu}

\maketitle

\end{document}
