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What is Bar Formation in Disc Galaxies Analysis about?

This study investigates the relationship between internal kinematics and environmental influences on bar formation in disc galaxies using data from the SDSS-IV MaNGA survey. The findings indicate that barred galaxies have higher stellar mass and lower angular momentum compared to unbarred ones, with bar formation primarily driven by internal gravitational instabilities, while external tidal interactions play a secondary role. The research provides observational validation for theoretical models of bar forma

Author

qetefirow98

Language

EN