Unveiling energy pathways in AGN accretion flows with the warm corona model for the soft excess.

MLA

Ballantyne, D. R., et al. “Unveiling Energy Pathways in AGN Accretion Flows with the Warm Corona Model for the Soft Excess.” Monthly Notices of the Royal Astronomical Society, vol. 530, no. 2, May 2024, pp. 1603–23. EBSCOhost, https://doi.org/10.1093/mnras/stae944.

APA

Ballantyne, D. R., Sudhakar, V., Fairfax, D., Bianchi, S., Czerny, B., De, R. A., De, M. B., Middei, R., Palit, B., Petrucci, P.-O., Różańska, A., & Ursini, F. (2024). Unveiling energy pathways in AGN accretion flows with the warm corona model for the soft excess. Monthly Notices of the Royal Astronomical Society, 530(2), 1603–1623. https://doi.org/10.1093/mnras/stae944

Chicago

Ballantyne, D R, V Sudhakar, D Fairfax, S Bianchi, B Czerny, Rosa, A De, Marco, B De, et al. 2024. “Unveiling Energy Pathways in AGN Accretion Flows with the Warm Corona Model for the Soft Excess.” Monthly Notices of the Royal Astronomical Society 530 (2): 1603–23. doi:10.1093/mnras/stae944.