Star-forming regions of NGC4395 with UV & Ha obs.

From our observations with the Ultra-Violet Imaging Telescope, we have compiled a catalog of 284 star-forming (SF) regions, out of which we could detect 120 SF regions in H{alpha} observations. Across the entire galaxy, we found the extinction-corrected star formation rate (SFR) in the far ultraviolet (UV) to range from 2.0x10^-5^M_{sun}_/yr to 1.5x10^-2^M_{sun}_/yr with a median of 3.0x10^-4^M_{sun}_/yr, and the age to lie in the range of ~1 to 98Myr with a median of 14Myr.

In H{alpha} we found the SFR to range from 7.2x10^-^6M_{sun}_/yr to 2.7x10^-2^M_{sun}_/yr with a median of 1.7x10^-4^M_{sun}_/yr, and the age to lie between 3 to 6Myr with a median of 5Myr. The stellar ages derived from H{alpha} show a gradual decline with galactocentric distance. We found three SF regions close to the center of NGC 4395 with high SFRs both from H{alpha} and UV, which could be attributed to feedback effects from the AGN.