Simulations of stellar disks in galaxies with non-Newtonian interactions

Astrophysics and Space Science

Volumn 226, Issue 1, 1995, Pages 51-72

  Griv, Evgeny ^a   Zhytnikov, Vadim V ^a  

^a NATIONAL CENTRAL UNIVERSITY   (Taiwan)

Author keywords

galaxies: dark matter; Galaxies: kinematics and dynamics

Indexed keywords

EID: 21844520570     PISSN: 0004640X     EISSN: 1572946X     Source Type: Journal    
DOI: 10.1007/BF00626899     Document Type: Article

References (48)

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4. The distribution of mass in spiral galaxies
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6. Effect of Population II Stars and Three-Dimensional Motion on Spiral Structure
7. Three-dimensional galaxy simulations
8. Observational constraints on driving mechanisms for spiral density waves
9. Non-Newtonian forces and the invisible mass problem
10. Exact vacuum solution to conformal Weyl gravity and galactic rotation curves
11. Solutions for the modified Newtonian dynamics field equation
12. Viscous evolution of self-gravitating galactic disks under modified Newtonian dynamics
13. A Numerical Study of the Stability of Flattened Galaxies: or, can Cold Galaxies Survive?
14. Alternatives to dark matter
15. The Kinematics of Spiral and Irregular Galaxies