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)
Zdroj:	Monthly Notices of the Royal Astronomical Society. Mar2019, Vol. 484 Issue 1, p196-203. 8p.
Databáze:	Academic Search Ultimate
Externí odkaz:	Zobrazit plný text záznamu