No CrossRef data available.
Article contents
Variable X-ray Absorption in NGC 4151
Published online by Cambridge University Press: 07 August 2017
Extract
The medium energy X-ray spectrum of the Seyfert galaxy NGC 4151 is characterised by a hard power-law continuum, a variable low-energy cut-off and iron line and edge features. Holt et al. (1980) found the spectral form below 4 keV to be incompatible with absorption in a uniform screen of cold gas and interpreted the apparent soft X-ray excess in terms of a partial covering model. However, recent observations point to a somewhat different description of the X-ray absorbing medium present in the nucleus of this galaxy.
- Type
- Part 3: X-rays and the Central Source
- Information
- Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 182 - 183
- Copyright
- Copyright © Kluwer 1989