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.
Roentgenstrahlung from the Universe
- Pub Date:
- February 1996
- Seyfert Galaxies: X-Ray Spectra