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              <text>Chemical processes in Solar-type star forming regions</text>
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              <text>How the chemical complexity evolves during the process leading to the formation of a Sun and its planetary system? Is the chemical richness of a Solar�like planetary system, at least partially, inherited from the earliest stages or is there a complete chemical reset? A powerful way to answering these questions is by comparing the chemical content in young protostars and primitive bodies of the Solar System, using astrochemistry as a tool. Yet, to do so, we need to fully understand the processes that govern the chemical evolution of a molecular cloud into a young planetary system.&#13;
The goal of the conference is to gather the actors of this intrinsically interdisciplinary endeavor: astronomers, chemists, and modelers. The recent  huge progresses in the three areas make the time ripe for these communities to join and ride this scientific wave.</text>
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              <text>Università degli Studi di Torino</text>
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              <text>2021</text>
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              <text>&lt;a rel="license" href="http://creativecommons.org/licenses/by-sa/4.0/"&gt;&lt;img alt="Licenza Creative Commons" style="border-width: 0;" src="https://i.creativecommons.org/l/by-sa/4.0/88x31.png" /&gt;&lt;/a&gt;&lt;br /&gt;Quest'opera è distribuita con Licenza &lt;a rel="license" href="http://creativecommons.org/licenses/by-sa/4.0/"&gt;Creative Commons Attribuzione - Condividi allo stesso modo 4.0 Internazionale&lt;/a&gt;.</text>
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              <text>ISBN: 9788875901844</text>
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              <text>Piero Ugliengo (ed.)</text>
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              <text>Claudio Codella (ed.)</text>
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      <name>interstellar ices</name>
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      <name>molecular complexity</name>
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      <name>molecular fractionation</name>
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