After having crossed an absorbing cloud, the intensity of a source, I, is received by the observer as I() = I, where is the optical depth of the cloud.
Let's connect to the physical parameters.
N : column densitya( : line absorption coefficient
: broadening functiona( =
l : lower level of the atomic transition
k : upper level of the atomic transition
: rest wavelength of the transition
g : statistical weight of the lower level
g : statistical weight of the upper level
a : spontaneous transition probability
f = upward oscillator strength