  The galaxy NGC6384 has been observed with an IPCS through H alpha and [NII]
narrow-band interference filters for direct imagery with the 2.6 m Byurakan
telescope. We studied main physical parameters of identified 98 HII regions,
their diameter and luminosity functions, as well [NII]/H alpha ratio
distribution. The integrated distribution function of the HII region diameters
can be well fitted by the exponential function. The characteristic diameter has
the value (Do = 217 pc) predicted for a galaxy of its measured absolute
luminosity. The luminosity function of HII regions has double power laws
profile with relatively shallow slope at low luminosities (a = - 0.4), an
abrupt turnover at log L(H alpha) = 38.75, and sharper slope at higher
luminosities (a = - 2.3). Correlation between luminosity and diameter of HII
regions confirms that in general they are constant density, radiation-bound
systems. [NII]/H alpha ratio data for HII regions show that there is a negative
radial gradient of [NII]/H alpha. In the central region of the galaxy, nitrogen
abundance is higher than in the periphery. The properties of the HII regions
population of this AGN galaxy does not differs significantly from the
properties of the HII regions population of the "normal" galaxies. Reexamining
the location of the type Ia SN 1971L in the galaxy, we confirm that it lies on
the spiral arm at about 8.6" far from the closest HII region #53 (F81). Such a
location can be taken as prove that the progenitor of this SN do not belong to
an old, evolved stellar population.
