Seyfert GalaxiesThese are AGN, where the host galaxy is still clearly visible beneath the dominating nuclear emission. They represent the closest and intrinsically faintest population of AGN. Their X-ray output is dominated by accretion. Depending on their optical properties, they are further classified into "type 1" (generally X-ray unobscured), and "type 2" (generally X-ray obscured) objects. They are believed to be the ultimate source of the X-ray Background. |
![]() 1H0707-495 | ![]() ESO 198-G24 | ![]() NGC 1068 | ![]() NGC 1365 | ![]() NGC 1808 |
![]() NGC 4258 | ![]() NGC 4258 | ![]() NGC 4258 | ![]() NGC 7582 | ![]() NGC1365 |
![]() NGC3516 | ![]() NGC4258 |