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☉.