Continuous Jets and Backflow Models for the Formation of W50/SS 433 in Magnetohydrodynamics Simulations
Author:
Funder
Kyushu University
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/abe5a1/pdf
Reference66 articles.
1. Publisher Correction: Very-high-energy particle acceleration powered by the jets of the microquasar SS 433
2. MAGNETOHYDRODYNAMIC SIMULATIONS OF A JET DRILLING AN H I CLOUD: SHOCK INDUCED FORMATION OF MOLECULAR CLOUDS AND JET BREAKUP
3. Beam models for SS 433
4. Detection of a Radio Bubble around the Ultraluminous X-Ray Source Holmberg IX X-1
5. Symmetry in the Changing Jets of SS 433 and Its True Distance from Us
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1. MHD lensing in inhomogeneous ISM for qualitative understanding of the morphology of supernova remnants;Astrophysics and Space Science;2024-08
2. Minimalist model of the W50/SS433 extended X-ray jet: Anisotropic wind with recollimation shocks;Astronomy & Astrophysics;2024-07-30
3. Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433;Science;2024-01-26
4. The high energy X-ray probe (HEX-P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binaries;Frontiers in Astronomy and Space Sciences;2023-12-22
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