Update paper.md

paper/paper.md

@@ -104,11 +104,8 @@ So far the code has been used to study a range of fundamental physics problems:
 - Growth of scalar hair around a Schwarzschild [@Clough:2019jpm] and a Kerr [@Bamber:2020bpu] black hole
 - Determining the relativistic drag forces on a Schwarzschild black hole moving through a cloud of scalar field dark matter [@Traykova:2021dua;@Traykova:2023qyv]
 
-![Formation of overdense tail of scalar dark matter behind a moving BH, due to dynamical friction \label{fig:friction}](Figures/friction.png){ width=45% }
-![The evolution of scalar clouds around black hole binaries in, the initial conditions were generated with a modified version of GRDzhadzha \label{fig:accretion}](Figures/accretion.png){ width=45% }
-
-![Formation of overdense tail of scalar dark matter behind a moving BH, due to dynamical friction \label{fig:friction}]<img src="Figures/friction.png" alt= “” width="200" height="200">
-![The evolution of scalar clouds around black hole binaries in, the initial conditions were generated with a modified version of GRDzhadzha \label{fig:accretion}]<img src="Figures/accretion.png" alt= “” width="200" height="200">
+![Formation of overdense tail of scalar dark matter behind a moving BH, due to dynamical friction \label{fig:friction}](Figures/friction.png){ width=15% }
+![The evolution of scalar clouds around black hole binaries in, the initial conditions were generated with a modified version of GRDzhadzha \label{fig:accretion}](Figures/accretion.png){ width=15% }
 
 
 - Studying the dynamical friction effects on a Kerr black hole (Magnus effect) [@Wang:inprep]