A Detailed Analysis of Star Formation and AGN Feedback Mechanism in Spiral Galaxy

Abstract

The manners in which stars form as well as how the Star Formation (SF) method is regulated in galaxies are the main themes in extragalactic astronomy. The SF analysis was examined by several prevailing researchers. But star formation in the cosmic environment with radiative and mechanical Active Galactic Nucleus (AGN) feedback mechanisms wasn’t investigated in most of the prevailing research works. A detailed analysis of SF and AGN feedback mechanisms in spiral galaxies is propounded in this paper. Assessing star formation and determining whether the feedback mechanism’s effect is positive or negative in spiral galaxies are the research’s main objectives. Moreover, this research analysis considers the J0313–1806 astronomical data for covering the cosmic environment in the SF of the spiral galaxy. For assessing the atomic, molecular, and Diffused Ionized Gas (DIG) values, hydrodynamic analysis is carried out. By utilizing the Silk-Elmegreen law, the relationship betwixt the Star Formation Rate (SFR) and the surface density of gas during SF in a spiral galaxy is assessed. According to the experimental results, the DIG has a higher fractional contribution, and the AGN feedback mechanism provides a positive effect on star formation.