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1994ApJ...431L...5C - Astrophys. J., 431, L5-L8 (1994/August-2)
Weak soft X-ray excesses need not result from the high-frequency tail of the optical/ultraviolet bump in active galactic nuclei.
CZERNY B. and ZYCKI P.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Accretion, Accretion Disks - Atomic Processes - Galaxies: Active - X-Rays: Galaxies
Simbad objects: 6
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