Connection between the Circumnuclear Star-Forming Regions and the active
  nuclei in NGC 1068
  In recent years, Circumnuclear Star Forming Regions (CNSFRs) have been
studied in different frequencies and telescopes, diverse studies about
connection between nuclear activity and star formation in the CNSFRs were doing
using optical data, IFS and models. We obtain data of the Seyfert 2 galaxy NGC
1068 at J band between 1.35-1.32$\mu$ using the 8.1m Gemini telescope and GNIRS
IFU mode. We found the radial velocity and intensity maps for
[FeII]$\lambda$12570, Pa$\beta$ $\lambda$12814 and FeII $\lambda$13201 lines of
all the components. The gas emission has a double origin associated with
photoionization by young stars or excitation by collisions, we found a high
influence of shocks produced by the jet. The intensity of Pa$\beta$ emission
show that this component is ionized by a younger cluster or more massive stars.
From the analysis of the velocity fields, the data related with the component
one of Pa$\beta$ are consistent with the presence of rotation which is
displaced from the maximum continuous, our observations may point to the
presence of a bar.
