English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

In recent years, Circumnuclear Star Forming Regions (CNSFRs) have beenstudied in different frequencies and telescopes, diverse studies aboutconnection between nuclear activity and star formation in the CNSFRs were doingusing optical data, IFS and models. We obtain data of the Seyfert 2 galaxy NGC1068 at J band between 1.35-1.32$\mu$ using the 8.1m Gemini telescope and GNIRSIFU mode. We found the radial velocity and intensity maps for[FeII]$\lambda$12570, Pa$\beta$ $\lambda$12814 and FeII $\lambda$13201 lines ofall the components. The gas emission has a double origin associated withphotoionization by young stars or excitation by collisions, we found a highinfluence of shocks produced by the jet. The intensity of Pa$\beta$ emissionshow 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 componentone of Pa$\beta$ are consistent with the presence of rotation which isdisplaced from the maximum continuous, our observations may point to thepresence of a bar.

Connection between the Circumnuclear Star-Forming Regions and the active nuclei in NGC 1068