Three-dimensional GRMHD Simulations of Neutron Star Jets
Neutron stars and black holes in X-ray binaries are observed to host strong collimated jets in the hard spectral state. Numerical simulations can act as a valuable tool in understanding the mechanisms behind jet formation and its properties. Although there have been significant efforts in understand...
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| Huvudupphov: | , |
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| Materialtyp: | Artigo |
| Språk: | Inglês |
| Utgiven: |
IOP Publishing
2024-01-01
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| Serie: | The Astrophysical Journal Letters |
| Ämnen: | |
| Länkar: | https://doi.org/10.3847/2041-8213/ad151f |
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