Numerical self-consistent stellar models of thin disks

DOI10.1051/0004-6361:20053176zbMath1105.85007arXivastro-ph/0505268OpenAlexW2078426761WikidataQ68850983 ScholiaQ68850983MaRDI QIDQ3410381

Patricio S. Letelier, Maximiliano Ujevic

Publication date: 27 November 2006

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0505268

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (3)

Exact relativistic magnetized haloes around rotating disks ⋮ Stability of general relativistic static thick disks: the isotropic Schwarzschild thick disk ⋮ Solving procedure for a 25-diagonal coefficient matrix: direct numerical solutions of the three-dimensional linear Fokker-Planck equation

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