Published November 28, 2025 | Version v1
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Merger of non-compact Binaries: Triggering Mechanisms and Merger Timescales of W UMa Contact Binaries (MESA-r23.05.1)

Authors/Creators

  • 1. Yunnan Observatories, Chinese Academy of Sciences

Description

These MESA inlist files were used to compute the stellar evolution models and merger timescales for the W UMa contact binaries studied in "Merger of non-compact Binaries: Triggering Mechanisms and Merger Timescales of W UMa Contact Binaries" (MESA-r23.05.1)

Files

Files (7.2 kB)

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md5:f516c5ad709318f353d837b72006d03e
2.9 kB Download
md5:603a4e8a402fa4c48f5d94fb124dcc19
1.0 kB Download
md5:5cd709d4f9a7ee177d52a5036a0bd43d
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