deletions | additions       diff --git a/section_Results_subsection_Enhanced_radio__.tex b/section_Results_subsection_Enhanced_radio__.tex  index 7b84606..490b8fe 100644  --- a/section_Results_subsection_Enhanced_radio__.tex  +++ b/section_Results_subsection_Enhanced_radio__.tex 
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From Figure 9 we observe as the pair velocity decreases -because of the closer interaction of the quasar pairs- the redshift (and thus the luminosity) increases. This is because accretion onto SMBHs releases energy that drives outflows which correlates to high luminosities seen in Figure 12.  The distribution of data points in Figure 10 indicate that we observe smaller wavelengths from the quasar pair as the separation between the quasars increases.  From Figure 11, we observe that as the separation between quasar pairs decreases the accretion rate, thus the luminosity of the core increases.