Protostellar cores formation in the collision of spherical and oblate clouds
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Publication:6544387
DOI10.1134/S1995080224010463zbMATH Open1543.76133MaRDI QIDQ6544387
Publication date: 27 May 2024
Published in: Lobachevskii Journal of Mathematics (Search for Journal in Brave)
ideal magnetohydrodynamicsconjugate gradient methodPoisson equationgravitational potentialmolecular cloudJacobi iteration methodChandrasekhar solution
Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Basic methods in fluid mechanics (76M99)
Cites Work
- Title not available (Why is that?)
- The stability of a spherical nebula.
- Modeling of density stratification and filamentous structure formation in molecular clouds after shock wave collision
- Riemann Solvers and Numerical Methods for Fluid Dynamics
- Comparison of Several Difference Schemes on 1D and 2D Test Problems for the Euler Equations
- Highly parallel structured adaptive mesh refinement using parallel language-based approaches
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