We observed twenty-eight Seyfert 2 galaxies with the Japanese X-ray satellite, Ginga, and found Seyfert 2 galaxies, in general, have the X-ray spectral characteristics of obscured Seyfert 1 nuclei. This results agrees with the predictions from the Unified Seyfert model proposed by Antonucci and Miller. However, among the observed Seyfert 2 galaxies, there are a few galaxies with no evidence of an obscuration, contrary to the general predictions of the unified model. We note that type 2 active galactic nuclei (AGN) will contribute to the Cosmic Diffuse X-ray Background, if the unified Seyfert model can be extended to the far distant AGN such as quasars.
Ginga observations of Seyfert galaxies
Advances in Space Research ; 13 , 12
1993-12-01
Miscellaneous
No indication
English
Ginga observations of Seyfert galaxies
Elsevier | 1993
|GINGA Observations of Seyfert Galaxies
British Library Conference Proceedings | 1993
|GINGA Observations of Seyfert Galaxies
Online Contents | 1993
|BBXRT and GINGA Observations of AGN
Online Contents | 1993
|BBXRT and GINGA Observations of AGN
British Library Conference Proceedings | 1993
|