<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>1390-0129</journal-id>
<journal-title><![CDATA[Revista Politécnica]]></journal-title>
<abbrev-journal-title><![CDATA[Rev Politéc. (Quito)]]></abbrev-journal-title>
<issn>1390-0129</issn>
<publisher>
<publisher-name><![CDATA[Escuela Politécnica Nacional]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1390-01292018000300023</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Cinemática y Masa dinámica de la Galaxia NGC 7331]]></article-title>
<article-title xml:lang="en"><![CDATA[Kinematics and Mass of the NGC 7331 Galaxy]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Armijos-Abendaño]]></surname>
<given-names><![CDATA[Jairo]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[López]]></surname>
<given-names><![CDATA[Ericson]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Llerena]]></surname>
<given-names><![CDATA[Mario]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Aldas]]></surname>
<given-names><![CDATA[Franklin]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Escuela Politécnica Nacional  ]]></institution>
<addr-line><![CDATA[ Quito]]></addr-line>
<country>Ecuador</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>07</month>
<year>2018</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>07</month>
<year>2018</year>
</pub-date>
<volume>41</volume>
<numero>2</numero>
<fpage>23</fpage>
<lpage>28</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://scielo.senescyt.gob.ec/scielo.php?script=sci_arttext&amp;pid=S1390-01292018000300023&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.senescyt.gob.ec/scielo.php?script=sci_abstract&amp;pid=S1390-01292018000300023&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.senescyt.gob.ec/scielo.php?script=sci_pdf&amp;pid=S1390-01292018000300023&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Resumen: Se llevó a cabo un estudio de la curva de rotación de la galaxia NGC 7331 situada a 14,7 Mpc de la Tierra. La curva de rotación se derivó usando observaciones radioastronómicas del monóxido de carbono (CO). La forma de la curva de rotación y las velocidades son muy similares a aquellas derivadas previamente, empleando datos de hidrógeno atómico, lo que sugiere la coexistencia de ambos elementos en las regiones estudiadas en NGC 7331. Se descubrió que el ensanchamiento de la línea de CO, transición 2-1, está dominado por efectos turbulentos del gas de CO antes que por efectos térmicos. Asimismo, se estudió el campo de velocidades de NGC 7331, lo que puso en evidencia la rotación de la galaxia en el sentido de las agujas del reloj. Finalmente, asumiendo una aproximación esférica para la forma de la galaxia se estimó una masa dinámica de 1,4E+10 masas solares para NGC 7331.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[Abstract: The study of the rotation curve of the galaxy NGC 7331, located at 13,870 Mpc from the Earth, was carried out. The rotation curve is obtained using radio astronomy observations of the carbon monoxide (CO). The shape of the rotation curve and the velocities are very similar to those derived from atomic hydrogen data, suggesting the coexistence of both elements in the studied regions of NGC 7331. We found that the CO (2-1) line broadening is dominated by turbulent effects rather than by thermal effects. The velocity field of the galaxy is studied as well, showing that the galaxy is rotating clockwise. Finally, assuming a spherical approximation for the galaxy shape, a dynamical mass of 1,4E+10 solar masses is estimated for NGC 7331.]]></p></abstract>
<kwd-group>
<kwd lng="es"><![CDATA[Radioastronomía]]></kwd>
<kwd lng="es"><![CDATA[galaxia]]></kwd>
<kwd lng="es"><![CDATA[curva de rotación]]></kwd>
<kwd lng="es"><![CDATA[masa galáctica]]></kwd>
<kwd lng="es"><![CDATA[gas molecular]]></kwd>
<kwd lng="en"><![CDATA[Radio astronomy]]></kwd>
<kwd lng="en"><![CDATA[galaxy]]></kwd>
<kwd lng="en"><![CDATA[rotation curve]]></kwd>
<kwd lng="en"><![CDATA[galactic mass]]></kwd>
<kwd lng="en"><![CDATA[molecular gas]]></kwd>
</kwd-group>
</article-meta>
</front><back>
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