  We estimated the angular momentum, $J$, of $720$ galaxies in the Local Volume
with distances $r < 12$ Mpc. The distribution of the average angular momentum
along the Hubble sequence has a maximum at the morphological type $T= 4$ (Sbc),
while the dispersion of the $J$-values for galaxies is minimal. Among the Local
Volume population, 27 elite spiral galaxies stand out, with an angular momentum
greater than 0.15 of the Milky Way, $J > 0.15 J_{MW}$, making the main
contribution ($ > 90\%$) to the total angular momentum of galaxies in the
considered volume. Using observational data on the kinematics and structure of
these galaxies, we determined the direction of their spins.
  We present the first map of the distribution of the spins of 27 nearby
massive spiral galaxies in the sky and note that their pattern does not exhibit
significant alignment with respect to the Local Sheet plane. The relationship
between the magnitude of the angular momentum and stellar mass of the local
galaxies is well represented by a power law with an exponent of ($5/3$) over an
interval of $6$ orders of magnitude of the mass of galaxies.
