Does the mid-infrared–hard X-ray luminosity relation for active galactic nuclei depend on Eddington ratio?
Autor: | Toba, Yoshiki1 (AUTHOR) toba@kusastro.kyoto-u.ac.jp, Ueda, Yoshihiro2 (AUTHOR), Matsuoka, Kenta3 (AUTHOR), Shidatsu, Megumi4 (AUTHOR), Nagao, Tohru5 (AUTHOR), Terashima, Yuichi4 (AUTHOR), Wang, Wei-Hao6 (AUTHOR), Chang, Yu-Yen6 (AUTHOR) |
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Zdroj: | Monthly Notices of the Royal Astronomical Society. Mar2019, Vol. 484 Issue 1, p196-203. 8p. |
Databáze: | Academic Search Ultimate |
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