X-RAY LUMINOUS IRAS GALAXIES

A sample of 14708 extragalactic IRAS sources selected from the Point S ource Catalog via statistical classification has been cross-correlated with the ROSAT All Sky Survey (Boller et al., 1992). 244 galaxies eme rge as being detected both by ROSAT and IRAS. The most interesting poi nt is the discovery of a dozen of ''normal'' spirals whose X-ray lumin osities reach nearly 10(43) erg s-1(0.1-2.4 keV), higher than previous detection limits of a few 10(41) erg s-1 (Stocke et al. 1991; Green, Anderson and Ward, 1992). We obtained optical spectra for nine of them , showing Seyfert spectra for three of the objects (thus previous mis- classifications), spectra close to LINERs for two further objects and normal IRAS galaxy spectra for the last four. In the case of ''normal' ' galaxies, the source of energy is not clear yet and could be related to the high rate of star formation likely to occur in the central reg ions or also to a low level active nucleus. The study of these objects is of interest to the nature of LINERs and, more generally, to possib le relations between AGN and starbursts (Sanders et al., 1988).