A ROSAT observation of the warm absorber in NGC 4051.
Abstract
The authors present a pointed ROSAT observation of the nearby low-luminosity Seyfert galaxy NGC 4051. The X-ray spectrum is modeled in terms of warm absorption. The properties of the warm gas are further constrained by taking into account the observed multi-wavelength spectral properties of NGC 4051. The warm-absorber intrinsic emission-line spectrum is discussed.
- Publication:
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Roentgenstrahlung from the Universe
- Pub Date:
- February 1996
- Bibcode:
- 1996rftu.proc..463K
- Keywords:
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- Seyfert Galaxies: X-Ray Spectra