The Baryonic Tully-Fisher
relation was extended to clusters hypothesizing that a0, the characteristic acceleration of the Modified
Newtonian Dynamics (MOND), depends on the mass of the system. Circular speeds
were calculated for systems with mass up to 1021 M☉. The relativistic impact on super massive systems
was considered using the extended Newtonian theory for gravitational bound
systems. The impact was an increase of the circular velocity for systems with
mass beyond ~1019 M☉.
Cite this paper
Quintero-Leyva, B. (2017). On the Extension of the Baryonic Tully-Fisher Relation to Galaxy Clusters and Super Massive-Cosmic Systems. Open Access Library Journal, 4, e3686. doi: http://dx.doi.org/10.4236/oalib.1103686.
Milgrom, M. (1983) A Modification of the Newtonian Dynamics as a Possible Alternative to the Hidden Mass Hypothesis. Astrophysical Journal , 270, 365-370.
Milgrom, M. (1983) A Modification of the Newtonian Dynamics. Implications for Galaxies. Astrophysical Journal , 270, 371-389.
Angus, G.W. and
McGaugh, S.S. (2007)
The Collision Velocity of the Bullet Cluster in Conventional and Modified
Dynamics. Monthly Notices of the Royal
Astronomical Society, 383, 417-423.
Nelson, A.H. (1988) On the Influence of Galaxy Magnetic
Fields on the Rotation Curves in the Outer Discs of Galaxies. Monthly Notices of the Royal Astronomical
Society, 233,115-121. https://doi.org/10.1093/mnras/233.1.115