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- W3022659308 abstract "The soft x ray properties of the Seyfert 2 galaxy NGC 1068 are a crucial test of the 'hidden Seyfert 1' model. It is important to determine whether the soft x rays come from the nucleus, or from a number of other possible regions in the circumnuclear starburst disk. We present preliminary results of a ROSAT HRI observation of NGC 1068 obtained during the verification phase. The fraction of x rays that can be attributed to the nucleus is about 70 percent so the 'soft x ray problem' remains. There is also significant diffuse x ray flux on arcminute scales, which may be related to the 'diffuse ionized medium' seen in optical emission lines, and the highly ionized Fe K(alpha) emission seen by BBXRT." @default.
- W3022659308 created "2020-05-13" @default.
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- W3022659308 date "1993-01-11" @default.
- W3022659308 modified "2023-09-27" @default.
- W3022659308 title "A ROSAT high resolution x ray image of NGC 1068" @default.
- W3022659308 hasPublicationYear "1993" @default.
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