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Inlists for paper: Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae

Vigna-Gómez, Alejandro; Justham, Stephen; Mandel, Ilya; de Mink, Selma E.; Podsiadlowski, Philipp


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    <subfield code="u">University of Chinese Academy of Sciences</subfield>
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    <subfield code="a">Vigna-Gómez, Alejandro</subfield>
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    <subfield code="a">&lt;p&gt;MESA (v10108) inlists for the models shown the &amp;quot;Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae&amp;quot; Letter (1903.02135). The inlists reproduce both the single and merger model.&lt;/p&gt;

&lt;p&gt;Contents:&lt;/p&gt;

&lt;p&gt;FiducialMergersPPISN.tar.gz&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;doubleMass&lt;/li&gt;
	&lt;li&gt;evolveMerged&lt;/li&gt;
	&lt;li&gt;evolveSingle&lt;/li&gt;
	&lt;li&gt;preMSmodel&lt;/li&gt;
	&lt;li&gt;README&lt;/li&gt;
&lt;/ul&gt;

&lt;p&gt;We also attach the single and merger MESA models at the moment where the central temperature is close to 10^9 K. These models where used to estimate the properties of the star, particularly core and envelope masses, as well as element abundances.&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;mergerAtLogTc9.data&lt;/li&gt;
	&lt;li&gt;singleAtLogTc9.data&lt;/li&gt;
&lt;/ul&gt;</subfield>
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