The Morphology of H{\alpha} emission in CALIFA galaxies
  We have determined the H{\alpha} emission line radial profiles for a sample
of 86 face-on galaxies observed in the CALIFA survey and analyzed with the
Pipe3D pipeline. From a visual analysis we propose a two step classification of
these profiles. Initially, they were divided in two classes with respect to the
maximum of the H{\alpha} emission: C (for central) profiles have the maximum
line emission at the galaxy center, whereas EX (for extended) profiles have the
maximum H{\alpha} emission outside the galaxy center. After, we divided the C
galaxies in two classes, CE and CL (where E and L stands here for 'early' and
'late'), through the value of $c_r$, the concentration index in the r-band. We
analyzed the profile class dependence of several galaxy parameters, as well as
examined the nature of line emission through the BPT diagram. We notice that
almost 75% of the sample is in the C class. Elliptical and S0 galaxies dominate
the CE class, with spiral galaxies being found mostly in the CL and EX classes.
We also notice that spirals in each of these classes have different properties,
with CL objects seeming less evolved than those in the EX class.
