A ROSAT observation of the warm absorber in NGC 4051.

Details A ROSAT observation of the warm absorber in NGC 4051. A ROSAT observation of the warm absorber in NGC 4051.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..463k&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 463 - 464

Astronomy and Astrophysics

Astrophysics

Seyfert Galaxies: X-Ray Spectra

Scientific paper

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.

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