================================================================================= "Low ionization nuclear emission-line regions (LINERs): Nature and Watermarks" Dr. Omaira Gonzalez-Martin Physics department, University of Crete, Greece ================================================================================= When: Wednesday, 4th of November of 2009 at 3:15 pm Where: 2nd Floor Seminar Room ================================================================================= Abstract: AGN emit over the entire electromagnetic spectrum and are widely believed to be powered by the accretion of matter onto a supermassive black hole (Rees 1984). Several families within the AGN category have been established from the observational point of view. Although their classification is sometimes misleading, it is widely believed that a unified model can explain them all under a single scenario (Antonucci 1993). However, this scheme needs to be further confirmed since there are several sub-classes of object that cannot be easily fitted into this scenario. One of the most intriguing cases are Low Ionization Nuclear Emission line Regions (LINERs). A long debate can be found in the literature proposing different physical processes as the main emission mechanism. This question become even more important since, according to their luminosity, they might be the link between active and normal galaxies. X-ray studies are one of the most powerful tools to unveil the true nature of LINERs. We have performed a careful study of the X-ray nuclear properties of a sample of 82 of these LINERs (Gonzalez-Martin et al. 2006; 2009a; 2009b). Around 90% of our sample shows evidences of AGN adding to this other indicators (radio flatness, UV variability and the presence of a broad Ha line). Therefore, we concluded that the vast majority of LINERs host an AGN as the main source of energy realized. However, the most important question is still open: Why are they different to other AGN families? I will describe two of the main differencies found between LINERs and their parent population of AGN, type 2 Seyfert: strong thermal emission and peculiar obscuration of the central source. Finally I would like to give you the main open outlines of this work and working progress on the field. =================================================================================