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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><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>
<b style="font-weight:normal;"
id="docs-internal-guid-93f70fca-e283-9ebd-2b18-be46556412d0">-- <br>
Secretaría de Ciencia y Técnica <br>
FCAGLP<br>
<br>
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</b></b>
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<b style="font-weight:normal;"
id="docs-internal-guid-31eaf2e4-72be-c014-8fde-9b6ce24bbc7c">
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:7pt;"><span style="font-size:18.666666666666664px;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:</span><span style="font-size:24px;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;"> </span><span style="font-size:18.666666666666664px;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;">Manel Perucho-Pla</span></p>
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;text-align:
justify;"><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;">Universidad de Valencia</span></p>
<br>
<p dir="ltr"
style="line-height:1.2;margin-top:0pt;margin-bottom:0pt;text-align:
justify;"><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;">Titulo:</span><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;"> </span><span style="font-size:16px;font-family:Verdana;color:#222222;background-color:#ffffff;font-weight:400;font-style:normal;font-variant:normal;text-decoration:underline;vertical-align:baseline;white-space:pre-wrap;">The complex dance between extragalactic jets and host galaxies.</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;">
</span><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;">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:#222222;background-color:#ffffff;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre-wrap;">Relativistic extragalactic jets are formed in the vicinity of supermassive black-holes in active galactic nuclei (AGN), and they propagate through and out of the host galaxy along tens and hundreds of kiloparsecs. These jets are among the most powerful astrophysical scenarios known, involving time-integrated energies of the order of 1.e60 erg and powers ranging from 1.e42 to 1.e47 erg/s. On the one hand, their supersonic flows trigger strong shocks that propagate through the interstellar medium of their host galaxies and eventually through the intracluster medium and, on the other hand, they are subject to the development of instabilities and to deceleration by entrainment. In my talk, I will show that jet evolution is not only affected by its
own properties, but also by those of the host galaxy, namely gas distribution and stellar population. I will also review several results that provide evidence for the host galaxy evolution being conditioned by the jet passage.</span></p>
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