Published August 12, 2026
| Version v1
Dataset
Open
Reproduction Package: Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry
Authors/Creators
-
1.
University of Amsterdam
Description
This is a reproduction package for the paper "Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry" by J. van den Eijnden and L. Kaper. It contains the data and scripts to check and re-do the analysis presented in the main paper.
Files
README.md
Files
(10.0 GB)
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md5:a088af80b91eb1bc3d2c55ba80f2a612
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md5:51720b80b2cd4584ef882a3d5476bddb
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3.9 MB | Preview Download |
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md5:5c03cd736e80500779d8582a4a60b70e
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265.5 kB | Preview Download |
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md5:87400e8f591fca0479ea0a0f443c68d0
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818.5 kB | Preview Download |
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md5:83ba563f1bcdc7fd76e4afa427147af5
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697.2 kB | Preview Download |
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md5:1cca0bff52ed1b09f4ee5abf42d08d03
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10.0 GB | Preview Download |
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md5:7ae4f4582eb9dca7daadbfbaf35c558b
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23.5 kB | Preview Download |
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md5:a37744ebeafe33fc3a1c0e06dbc9b866
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5.0 MB | Preview Download |
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md5:9d7c4a65d685a5b8432867af4714b08a
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9.8 MB | Preview Download |
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md5:becf983b62a05c9b512d5eeda8d5541d
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1.1 MB | Preview Download |
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md5:252a87a5b68f62a7bede46745a3f6635
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4.0 kB | Preview Download |
Additional details
Related works
- Is supplement to
- Preprint: 10.48550/arXiv.2608.05946 (DOI)
- Journal article: 10.1093/mnras/stag1539 (DOI)
Funding
Software
- Repository URL
- https://github.com/jvandeneijnden/MisalignedBowshocks/
- Programming language
- Python , Jupyter Notebook