  H-alpha and continuum images are presented for 27 nearby early-type(Sa-Sab)
spiral galaxies. Contrary to popular perception, the images reveal copious
massive star formation in some of these galaxies. A determination of the
H-alpha morphology and a measure of the H-alpha luminosity suggests that
early-type spirals can be classified into two broad categories based on the
luminosity of largest HII region in the disk. The first category includes
galaxies for which the individual HII regions have L(H-alpha) < 10^(39) erg/s.
Most of the category 1 galaxies appear to be morphologically undisturbed, but
show a wide diversity in nuclear H-alpha properties. The second category
includes galaxies which have at least one HII region in the disk with
L(H-alpha) > 10^(39) erg/s. All category 2 galaxies show either prominent dust
lanes or other morphological peculiarities such as tidal tails which suggests
that the anomalously luminous HII regions in category 2 galaxies may have
formed as a result of a recent interaction. The observations, which are part of
an on-going H-alpha survey, reveal early-type spirals to be a heterogeneous
class of galaxies that are evolving in the current epoch.
  We have also identified some systematic differences between the
classifications of spiral galaxies in the Second General Catalog (RC2) and the
Revised Shapley-Ames Catalog (RSA) which may be traced to subtle variations in
the application of the criteria used for classifying spiral galaxies. An
examination of earlier studies suggests that perceptions concerning the Hubble
type dependence of star formation rates among spiral galaxies depends on the
choice of catalog.
