The Astrophysical Journal · 1984 · 60 citations · 0 references
Natural SciencesAstronomyPhysicsAstrophysicsSpectroscopyX-ray AstronomyAbsorption SpectroscopyHigh-energy Astrophysical SourcesHigh-energy AstrophysicsX-ray SpectroscopyAbsorption SpectraAstronomical ObservationEmission SpectraSoft X-ray AstronomyX-ray Absorption SpectroscopyX-ray Emission LinesX-ray Line EmissionX-ray Spectra
An absorption feature appears at 600 eV and extends to higher energies by 50 - 100 eV in a spectrum that covers the range from 0.38 to 1.6 keV obtained with the objective grating spectrometer on the Einstein Observatory. The spectrum can be fitted by a single absorption edge or trough plus two power laws with slopes that are consistent with simultaneous measurements of the 2 - 10 keV flux. The absence of a low-energy cutoff is consistent with a neutral column density of N<SUB>H I</SUB> ≡ 4×10<SUP>20</SUP> cm<SUP>-2</SUP>. Absorption by ionized oxygen is by far the most likely explanation of the sharp feature, and possible detailed interpretations are discussed.