We have obtained hard X-ray spectra of four luminous IRAS galaxies, which were selected on the basis of their optical polarized broad lines. We have found prominent Fe K line emission from IRAS 20210+1121, suggesting that its observed X-ray continuum is scattered emission from a completely blocked AGN. The X-ray-[OIII]lambda 5007 ratios of our sources are in the range of moderately or heavily absorbed Seyfert 2s. (C) 2000 COSPAR. Published by Elsevier Science Ltd.
Ueno, S., Ward, M.j., O'Brien, P.t., Stirpe, G.m., Matt, G. (2000). BeppoSAX observations of luminous IRAS galaxies. ADVANCES IN SPACE RESEARCH, 25(3-4), 823-826 [10.1016/S0273-1177(99)00848-0].