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astro-ph.HE2026
Bolometric correction factor and radiative efficiency for the super-Eddington accretion flow in tidal disruption events
Yongxin Wu, Erlin Qiao, Xuan Fang +3
The estimate of the bolometric luminosity and the radiative efficiency are two key aspects for understanding the properties of the accretion flow around a supermassive black hole (…
astro-ph.HE2026
Radiation hydrodynamic simulations for the origin of quasi-periodic oscillations for accretion onto supermassive black holes
Yiyang Lin, Erlin Qiao, Jifeng Liu +2
Quasi-periodic oscillation (QPO) has been detected in several accreting supermassive black hole (SMBH) systems, including active galactic nuclei (AGNs) and tidal disruption events…
astro-ph.HE2025
Early evolution of super-Eddington accretion flow in tidal disruption events
Erlin Qiao, Yongxin Wu, Yiyang Lin +5
Tidal disruption events (TDEs) are luminous black hole (BH) transient sources, which are detected mainly in X-ray and optical bands. It is generally believed that the X-ray emissio…