Aggarwal, Y. (2024). Evidence that Eddington ratio depends upon a supermassive black hole's mass and redshift: Implications for radiative efficiency.
Chicago Style (17th ed.) CitationAggarwal, Yash. Evidence That Eddington Ratio Depends upon a Supermassive Black Hole's Mass and Redshift: Implications for Radiative Efficiency. 2024.
MLA (9th ed.) CitationAggarwal, Yash. Evidence That Eddington Ratio Depends upon a Supermassive Black Hole's Mass and Redshift: Implications for Radiative Efficiency. 2024.
Warning: These citations may not always be 100% accurate.