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<p>Hola a todos,<br>
<br>
<b style="font-weight:normal;"
id="docs-internal-guid-93f70fca-e283-9ebd-2b18-be46556412d0">Les
recordamos que hoy tendremos el siguiente seminario a las </b><span
style="font-weight:normal;">13</span><span
style="font-weight:normal;">:00 </span><b
style="font-weight:normal;"
id="docs-internal-guid-93f70fca-e283-9ebd-2b18-be46556412d0">hs.
en el Salón Meridiano. </b>Los esperamos 15 minutos antes del
Seminario con café y galletitas. <br>
</p>
<b style="font-weight:normal;"
id="docs-internal-guid-93f70fca-e283-9ebd-2b18-be46556412d0">-- </b><b
style="font-weight:normal;"
id="docs-internal-guid-93f70fca-e283-9ebd-2b18-be46556412d0"><br>
Secretaría de Ciencia y Técnica </b><b
style="font-weight:normal;"
id="docs-internal-guid-93f70fca-e283-9ebd-2b18-be46556412d0"><br>
FCAGLP</b><b style="font-weight:normal;"
id="docs-internal-guid-93f70fca-e283-9ebd-2b18-be46556412d0"><b><br>
-----------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------<br>
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<b style="font-weight:normal;"
id="docs-internal-guid-8ab74edd-00d5-da93-b072-45021be516c8">
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:16px;font-family:Verdana;color:#000000;background-color:transparent;font-weight:700;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;">Seminario: Arianna Cortesi</span></p>
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:14.666666666666666px;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;">Universidade de Sao Paulo, Instituto de Astronomia, Geofisica e Ciencias Atmosfericas (IAG) Cidade Universitaria Rua do Matao, Sao Paulo - SP, Brazil</span></p>
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style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;"><br>
</div>
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:14.666666666666666px;font-family:Verdana;color:#000000;background-color:transparent;font-weight:700;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;">TÍTULO</span></p>
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;text-align:
justify;"><span style="font-size:14.666666666666666px;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;">Recovering the origin of Lenticular Galaxies from stellar kinematics and multi-wavelengths surveys.</span></p>
<div dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;"><br>
</div>
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:14.666666666666666px;font-family:Verdana;color:#000000;background-color:transparent;font-weight:700;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;">RESUMEN</span></p>
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;text-align:
justify;"><span style="font-size:14.666666666666666px;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;">Recent results from IFU surveys, as SAURON and Califa, changed our view of galaxy classification, proposing to use the kinematic balance between rotation and random motion in a galaxy, in order to classify galaxies into fast and slow rotators; with some of the fast rotators presenting spiral arms. In this new view, lenticular galaxies, which traditionally fall at the apex of the Hubble tuning fork, between elliptical and spiral galaxies, will naturally fall in the fast-rotator group. It is now to be understood if all fast rotators are lenticular galaxies or whether there are different path to create fast rotators and even lenticular galaxies. In this talk I will present results from planetary nebulae and globular clusters kinematics to tackle this issue. I will show some attempt to use multi-band images to identify parameter that can be use to classify galaxies and I will introduce a new Brazilian-Spanish survey (J-PAS), that will observe the northern sky in 56 filters, and the south and north hemisphere in 12 filters (S-PLUS and J-PLUS).</span></p>
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id="docs-internal-guid-75cda3d2-00d2-ba60-b549-f6ab27013b8a"><span style="font-size:16px;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;"></span></b>
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