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

has been cited by the following article:

• TITLE: On the Extension of the Baryonic Tully-Fisher Relation to Galaxy Clusters and Super Massive-Cosmic Systems

  AUTHORS: Barbaro Quintero-Leyva

  KEYWORDS: Dark Matter, Dark Energy, Galaxies: Kinematics and Dynamics, Clusters, Cosmology

  JOURNAL NAME: Open Access Library Journal, Vol.4 No.6, June 20, 2017

  ABSTRACT: 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☉.