2004A&A...413..921D

We report on the analysis of a BeppoSAX observation of IRAS 13197-1627. The complexity of the broad band (0.3-100keV) spectrum of the source prevents us from selecting from two possible best-fit models, i.e. one based on a partial covering and the other on a reflection dominated scenario. Whatever the best fit model, the data imply that: 1) the primary spectrum is heavily obscured by at least two absorbers with column densities of the order of 5x10²³cm^–2 and ≥2x10²⁴cm^–2; 2) the intrinsic 2-10keV luminosity of the source is at least ∼2x10⁴⁴erg/s thus making IRAS 13197-1627 a type-II QSO (more precisely a type 1.8 QSO) rather than a Seyfert 1.8 galaxy as previously classified. Furthermore, there is marginal evidence of an absorption line at E∼7.5keV suggesting a possible outflow with v∼0.1c similar to recent findings on other QSOs and Seyferts.