%0 Journal Article
%T On the Extension of the Baryonic Tully-Fisher Relation to Galaxy Clusters and Super Massive-Cosmic Systems
%A Barbaro Quintero-Leyva
%J Open Access Library Journal
%V 4
%N 6
%P 1-10
%@ 2333-9721
%D 2017
%I Open Access Library
%R 10.4236/oalib.1103686
%X <div style="text-align:justify;">
	<span style="line-height:1.5;">The Baryonic Tully-Fisher
relation was extended to clusters hypothesizing that </span><i style="line-height:1.5;">a</i><sub>0</sub><span style="line-height:1.5;">, the characteristic acceleration of the Modified
Newtonian Dynamics (MOND), depends on the mass of the system. Circular speeds
were calculated for systems with mass</span><span style="line-height:1.5;"> up to 10</span><sup>21</sup><span style="line-height:1.5;"> M</span><sub>¨‘</sub><span style="line-height:1.5;">. 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 ~10</span><sup>19</sup><span style="line-height:1.5;"> M</span><sub>¨‘</sub><span style="line-height:1.5;">.</span>
</div>
%K Dark Matter
%K Dark Energy
%K Galaxies: Kinematics and Dynamics
%K Clusters
%K Cosmology
%U http://www.oalib.com/paper/5286754