X-ray absorption in Seyfert 2 galaxies

We have studied the correlation among X-ray absorption, optical reddening and nuclear dust morphology in Seyfert 2 galaxies. Two main conclusions emerge (i) the Balmer decrement and the amount of X-ray absorption are anticorrelated over a wide range of column density, 10<SUP>21</SUP><~N<SUB>H</SUB><~10<SUP>24</SUP>cm<SUP>- 2</SUP> - the correlation no longer applies to Compton-thick objects (N<SUB>H</SUB>>~10<SUP>24</SUP>cm<SUP>-2</SUP>), although they span a comparable range in Balmer decrement; (ii) Compton-thin Seyfert 2s seem to prefer nuclear environments, which are rich in dust on scales of hundreds of parsecs. On the other hand, Compton-thick Seyferts indifferently exhibit `dust-poor' and `dust-rich' environments. These results support an extension of the Seyfert unification scenario (as recently proposed by Matt), where Compton-thick Seyfert 2s are observed through compact `torii', whereas Compton-thin ones are obscured by dust on much larger scales.