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<oembed><version>1.0</version><provider_name>Arbeitsgemeinschaft der Universit&#xE4;tsverlage</provider_name><provider_url>https://universitaetsverlage.eu</provider_url><author_name>XMLRPC</author_name><author_url>https://universitaetsverlage.eu/author/xmlrpc/</author_url><title>Communications in Asteroseismology, Volume 158/2009 - Arbeitsgemeinschaft der Universit&#xE4;tsverlage</title><type>rich</type><width>600</width><height>338</height><html>&lt;blockquote class="wp-embedded-content"&gt;&lt;a href="https://universitaetsverlage.eu/bucher-e-books/titel/communications-in-asteroseismology-volume-158-2009-ebook/"&gt;Communications in Asteroseismology, Volume 158/2009&lt;/a&gt;&lt;/blockquote&gt;
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&lt;/script&gt;&lt;iframe sandbox="allow-scripts" security="restricted" src="https://universitaetsverlage.eu/bucher-e-books/titel/communications-in-asteroseismology-volume-158-2009-ebook/embed/" width="600" height="338" title="&#x201E;Communications in Asteroseismology, Volume 158/2009&#x201C; &#x2014; Arbeitsgemeinschaft der Universit&#xE4;tsverlage" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"&gt;&lt;/iframe&gt;</html><thumbnail_url>https://universitaetsverlage.eu/wp-content/uploads/asolmerce/image-9783700166245.jpg</thumbnail_url><thumbnail_width>354</thumbnail_width><thumbnail_height>549</thumbnail_height><description>This colloquium was the 38th Li&#x2018;ege International Astrophysical Colloquium(38thLIAC -http://www.ago.ulg.ac.be/APub/Colloques/Liac38);it was also held under the auspices of the European Helio- and Asteroseismology Network(HELAS - http://www.helas-eu.org/), the CoRoT Evolution and Seismic Tools Activity(CoRoT/ESTA - http://www.astro.up.pt/esta/) and the Belgian Asteroseismology Group(BAG - http://www.asteroseismology.be). The first part of the conference was devoted to the internal structure of massive stars with session 1 dealing with the theoretical aspects of non standard physical processes while session 2 presented the challenges met in stellar modelling when introducing these physical processes. Session 3 was a &#x201C;state of the art&#x201D; in atmospheres, mass loss and stellar winds in massive stars. Session 4 presented the pulsation observations in massive stars while session 5 discussed the asteroseismic signatures of the physical processes involved in their internal structure. A final session 6 was essentially focused on the interpretation of the asteroseismic observations of ground-based, MOST and CoRoT targets.</description></oembed>
