Rotation curves of spiral galaxies: Influence of magnetic fields and energy flows

Acta Physica Polonica B

Volumn 35, Issue 10, 2004, Pages 2493-2501

  Kutschera, M ^a,b   Jalocha, J ^a  

^a JAGIELLONIAN UNIVERSITY   (Poland)

^b INSTITUTE OF NUCLEAR PHYSICS   (Poland)

Author keywords

[No Author keywords available]

Indexed keywords

ACCELERATION; ASTROPHYSICS; GRAVITATION; MAGNETIC FIELD EFFECTS; PROBLEM SOLVING; ROTATION;

KEPLERIAN METHODS; NON-NEWTONIAN GRAVITATIONAL ACCELERATIONS; SCHWARZSCHILD METRIC; SPIRAL GALAXIES;

GALAXIES;

EID: 7044235233     PISSN: 05874254     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Article

References (10)

1. P.C. Vaidya, Nature 171, 260 (1953).
2. A.J. Romanowsky, N.G. Douglas, M. Arnaboldi, K. Kuiken, M.R. Merrifield, N.R. Napolitano, M. Capaccioli, K.C. Freeman, Science 301, 1696 (2003).
3. A.H. Nelson, Mon. Not. R. Astron. Soc. 233, 115 (1988).
4. E. Battaner, J.L. Garrido, M. Membrado, E. Florido, Nature 360, 652 (1992).
5. R.C. Tolman, Relativity, Thermodynamics and Cosmology, Oxford, Clarendon Press, 1934.
6. R.W. Lindquist, R.A. Schwartz, Phys. Rev. 137, B1364 (1965).
7. M. Milgrom, Astrophys. J. 270, 356 (1983).
8. M. Milgrom, R.H. Sanders, Astrophys. J. 599, L25 (2003).
9. K. Lake, Phys. Rev. Lett. 92, 051101 (2003).
10. F.J. Sanchez-Salcedo, M. Reyes-Ruiz, astro-ph/0402022.