Probable Model for Cumulative Jet Formation in Process of Relativistic Emission from Black Hole by the Example of Merely Gas-Dynamic Mechanism
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Publisher
Springer Nature Singapore
Link
https://link.springer.com/content/pdf/10.1007/978-981-97-1872-6_26
Reference19 articles.
1. Koide, S., Shibata, K., Kudoh, T.: Relativistic Jet formation from black hole magnetized accretion disks: method, tests, and applications of a general relativistic magnetohydrodynamic numerical code. ApJ 522, 727 (1999)
2. Meliani, Z., Sauty, C., Tsinganos, K., Trussoni, E., Cayatte, V.: Relativistic spine jets from Schwarzschild black holes Application to AGN radio-loud sources. A&A 521, A67 (2010)
3. Contopoulos, I., Gabuzda, D., Kylafis, N.: The Formation and Disruption of Black Hole Jets. Springer, Cham (2014). https://doi.org/10.1007/978-3-319-10356-3
4. Beall, J.H.: A review of Astrophysical Jets. Acta Polytechnica CTU Proceedings 1(1), 259–264 (2014)
5. Beall, J. H.: A Review of Astrophysical Jets. Proceedings of Science 58 (2015)
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