Cite
Model of a "Warm Corona" as the origin of the soft X-ray excess of active galactic nuclei.
MLA
Kawanaka, Norita, and Shin Mineshige. “Model of a ‘Warm Corona’ as the Origin of the Soft X-Ray Excess of Active Galactic Nuclei.” Publications of the Astronomical Society of Japan, vol. 76, no. 2, Apr. 2024, pp. 306–15. EBSCOhost, https://doi.org/10.1093/pasj/psae012.
APA
Kawanaka, N., & Mineshige, S. (2024). Model of a “Warm Corona” as the origin of the soft X-ray excess of active galactic nuclei. Publications of the Astronomical Society of Japan, 76(2), 306–315. https://doi.org/10.1093/pasj/psae012
Chicago
Kawanaka, Norita, and Shin Mineshige. 2024. “Model of a ‘Warm Corona’ as the Origin of the Soft X-Ray Excess of Active Galactic Nuclei.” Publications of the Astronomical Society of Japan 76 (2): 306–15. doi:10.1093/pasj/psae012.