Iras-allsky

Limits on the X-ray emission from several hyperluminous IRAS galaxies

October 1998 • 1998MNRAS.300L...7W

Authors • Wilman, R. J. • Fabian, A. C. • Cutri, R. M. • Crawford, C. S. • Brandt, W. N.

Abstract • We report long, pointed ROSAT HRI observations of the hyperluminous galaxies IRAS F00235+1024, F12514+1027, F14481+4454 and F14537+1950. Two of them are optically classified as Seyfert-like. No X-ray sources are detected at the positions of any of the objects, with a mean upper limit L_X/L_Bol~=2.3x10^-4. This indicates that any active nuclei are either atypically weak at X-ray wavelengths or obscured by column densities N_H>10^23cm^-2. They differ markedly from `ordinary' Seyfert 2 galaxies, bearing a closer resemblance in the soft X-ray band to composite Seyfert 2 galaxies or to some types of starburst.

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Roc Cutri

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