Aggarwal, Y. (2024). Evidence that Eddington ratio depends upon a supermassive black hole's mass and redshift: Implications for radiative efficiency.
Citazione stile Chigago Style (17a edizione)Aggarwal, Yash. Evidence That Eddington Ratio Depends upon a Supermassive Black Hole's Mass and Redshift: Implications for Radiative Efficiency. 2024.
Citatione MLA (9a ed.)Aggarwal, Yash. Evidence That Eddington Ratio Depends upon a Supermassive Black Hole's Mass and Redshift: Implications for Radiative Efficiency. 2024.
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