Astronomy and Astrophysics · 2007 · 13 citations · 38 references
Natural SciencesAstronomyPhysicsAstrophysicsObservational AstronomyX-ray AstronomyExtragalactic X-ray SourcesGalactic X-ray SourcesX-ray Data AnalysisX-ray TimingEddington LimitPower Spectral DensityPower Spectral Density AnalysisSeyfert GalaxiesSpectral-timing AnalysisTwo-component Mixing ModelsX-ray Line EmissionX-ray Variability Amplitude
Context.The Seyfert 1.8 galaxy ESO 113-G010 had been observed for the first time above 2 keV by XMM-Newton during a short exposure (~4 ks) in May 2001. In addition to a significant soft X-ray excess, it showed one of the strongest (in EW) redshifted Fe Kα lines, at 5.4 keV.
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Abundances of the elements: Meteoritic and solar
Edward Anders, N. Grevesse · Geochimica et Cosmochimica Acta · 1989 · 10.5K citations
J. M. Dickey, Felix J. Lockman · Annual Review of Astronomy and Astrophysics · 1990 · 4.6K citations
On the Absorption of X‐Rays in the Interstellar Medium
The Astrophysical Journal · 2000 · 3.9K citations · Full text
Natural Sciences, Astronomy, Physics +14
The European Photon Imaging Camera on XMM-Newton: The pn-CCD camera
L. Strüder, U. G. Briel, K. Dennerl et al. · Astronomy and Astrophysics · 2001 · 3K citations · Full text
Natural Sciences, Astronomy, Physics +17