Kinematic Signatures of Bulges Correlate with Bulge Morphologies and
  S\'ersic Index
  We use the Marcario Low Resolution Spectrograph (LRS) at the
Hobby-Eberly-Telescope (HET) to study the kinematics of pseudobulges and
classical bulges in the nearby universe. We present major-axis rotational
velocities, velocity dispersions, and h3 and h4 moments derived from
high-resolution (sigma ~ 39 km/s) spectra for 45 S0 to Sc galaxies; for 27 of
the galaxies we also present minor axis data. We combine our kinematics with
bulge-to-disk decompositions. We demonstrate for the first time that purely
kinematic diagnostics of the bulge dichotomy agree systematically with those
based on S\'ersic index. Low S\'ersic index bulges have both increased
rotational support (higher v/sigma values) and on average lower central
velocity dispersions. Furthermore, we confirm that the same correlation also
holds when visual morphologies are used to diagnose bulge type. The previously
noted trend of photometrically flattened bulges to have shallower velocity
dispersion profiles turns to be significant and systematic if the S\'ersic
index is used to distinguish between pseudobulges and classical bulges. The
correlation between h3 and v/sigma observed in elliptical galaxies is also
observed in intermediate type galaxies, irrespective of bulge type. Finally, we
present evidence for formerly undetected counter rotation in the two systems
NGC 3945 and NGC 4736.
  Based on observations obtained with the Hobby-Eberly Telescope, which is a
joint project of the University of Texas at Austin, the Pennsylvania State
University, Stanford University, Ludwig-Maximilians-Universit\"at M\"unchen,
and Georg-August-Universit\"at G\"ottingen.
