Iron K-alpha line profiles computed in the Ruffini-Argüelles-Rueda fermionic dark matter metric show that the most compact non-rotating cores mimic high-spin Kerr lines and can reproduce MCG-06-30-15.
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Iron K$\alpha$ signatures from accretion disks around fermionic dark matter cores
Iron K-alpha line profiles computed in the Ruffini-Argüelles-Rueda fermionic dark matter metric show that the most compact non-rotating cores mimic high-spin Kerr lines and can reproduce MCG-06-30-15.