Dataset Open Access

A new route towards merging massive black holes

Marchant, Pablo; Langer, Norbert; Podsiadlowski, Philipp; Tauris, Thomas M.; Moriya, Takashi J.


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    <subfield code="a">&lt;p&gt;MESA inlists, run_star_extras, and data associated with &lt;a href="https://ui.adsabs.harvard.edu/?#abs/2016A&amp;amp;A...588A..50M"&gt;Marchant et al. (2016)&lt;/a&gt;. MESA version 8118.&lt;/p&gt;

&lt;p&gt;Publication DOI:&amp;nbsp;&lt;a href="https://doi.org/10.1051/0004-6361/201628133"&gt;10.1051/0004-6361/201628133&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;Files are also available in a gihub repository &lt;a href="https://github.com/orlox/mesa_input_data/tree/master/2016_double_bh"&gt;here&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;Upload includes post-processed simulation output in the files Z04.tar.xz (for Z=Zsun/4), Z10.tar.xz&amp;nbsp;(for Z=Zsun/10),&amp;nbsp;Z20.tar.xz&amp;nbsp;(for Z=Zsun/20) and&amp;nbsp;Z50.tar.xz&amp;nbsp;(for Z=Zsun/50). Each folder inside the archive corresponds to a single MESA simulation, with the name indicating the value of log10(M_1), q=M2/M1&amp;nbsp;and the orbital period in days. For example, the directory 1.6_1.00_0.90 corresponds to the simulation with log10(M1)=1.6, M2/M1=1 and Porb=0.9 days. Each folder is also a MESA template folder, containing all input files neccesary to reproduce that individual simulation.&lt;/p&gt;</subfield>
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