In SI units you have
$$\alpha=\frac{e^2}{4 \pi \epsilon_0 \hbar c} \simeq 1/137,$$
which is dimensionless. This is the Sommerfeld fine structure constant describing, in natural units, the interaction strength of charged particles due to their electromagnetic interaction (##e\simeq 1.6 \cdot 10^{-19} \mathrm{C}## is the charge of a proton, ##\hbar## is Planck's modified constant, and ##c## the speed of light, ##\epsilon_0## is an artifact of the "ugly" SI units, which are made for practical purposes rather than to expose the beauties of a consistent relativistic formulation of classical and quantum electrodynamics).
In modern high-energy physics, rationalized Gaussian (also called Heaviside-Lorentz) units are used, which brings the full symmetry of space and time and the correct relativistic dimensions of the electromagnetic field forward (electric and magnetic field components having the same unit). In addition, theoreticans have a hard time with their math anyway, and thus reduce the effort further by choosing "natural units", measuring angular momenta, actions, etc. in units of ##\hbar##. Thus effectively they set ##\hbar=1##. Then, as space and time are very much more symmetric in relativistic than in Newtonian physics, it nearly doesn't make sense to measure them in different units. This is the more true since also in the SI units the speed of light is just a conversion factor with a once-and-for all fixed value. So you can as well set ##c=1## and measure velocities in units of ##c##. This implies that energies and momenta have the same unit, usually using MeV or GeV, which is convenient when working in high-energy physics as at the LHC. Also lengths and times have the same unit. Here a convenient scale is fermi (or femtometer, which is ##10^{-15} \;\mathrm{m}##).
To convert back to usual units, one simply has to do some dimensional analysis of the quantity in question and use the relation ##\hbar c \simeq 0.197 \;\text{MeV} \; \text{fm}##.
Then you need to remember just one more thing: Cross sections are usually given in milli-barns. Then you just have to remember that ##10 \; \mathrm{mb} = 1 \; \mathrm{fm}^2=10^{-30} \; \mathrm{mb}##.