Newtonian stellar models.

DOI10.1016/S0003-4916(03)00130-1zbMath1045.85001arXivastro-ph/0211628MaRDI QIDQ1415308

J. Mark Heinzle, Claes Uggla

Publication date: 3 December 2003

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0211628

zbMATH Keywords

polytropic equation of statestatic perfect fluidsdynamical stellar models

Mathematics Subject Classification ID

Dynamical systems in fluid mechanics, oceanography and meteorology (37N10) Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (11)

(In)finite extent of stationary perfect fluids in Newtonian theory ⋮ Static self-gravitating Newtonian elastic balls ⋮ Stability of rotating gaseous stars ⋮ The uniqueness of the slowly uniformly rotating supermassive star for a given total mass ⋮ On the asymptotic behavior of static perfect fluids ⋮ Multi-body spherically symmetric steady states of Newtonian self-gravitating elastic matter ⋮ Self-gravitating stationary spherically symmetric systems in relativistic galactic dynamics ⋮ On the fluid ball conjecture ⋮ Static perfect fluids with Pant-Sah equations of state ⋮ Self-Gravitating Newtonian Disks Revisited ⋮ Stabilization and stability for the spherically symmetric Navier-Stokes-Poisson system

Cites Work

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• Applications of centre manifold theory
• On spherically symmetric stellar models in general relativity
• Existence and properties of spherically symmetric static fluid bodies with a given equation of state
• Dynamics of spatially homogeneous solutions of the Einstein-Vlasov equations which are locally rotationally symmetric
• On static stars in Newtonian gravity and Lane-Emden type equations
• General relativistic stars: Polytropic equations of state

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