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A new route towards merging massive black holes

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

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<oai_dc:dc xmlns:dc="" xmlns:oai_dc="" xmlns:xsi="" xsi:schemaLocation="">
  <dc:creator>Marchant, Pablo</dc:creator>
  <dc:creator>Langer, Norbert</dc:creator>
  <dc:creator>Podsiadlowski, Philipp</dc:creator>
  <dc:creator>Tauris, Thomas M.</dc:creator>
  <dc:creator>Moriya, Takashi J.</dc:creator>
  <dc:description>MESA inlists, run_star_extras, and data associated with Marchant et al. (2016). MESA version 8118.

Publication DOI: 10.1051/0004-6361/201628133

Files are also available in a gihub repository here

Upload includes post-processed simulation output in the files Z04.tar.xz (for Z=Zsun/4), Z10.tar.xz (for Z=Zsun/10), Z20.tar.xz (for Z=Zsun/20) and Z50.tar.xz (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 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.</dc:description>
  <dc:source>Astronomy &amp; Astrophysics Volume 588 id.A50, 13 pp. (2016)</dc:source>
  <dc:title>A new route towards merging massive black holes</dc:title>
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