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- W3100659219 endingPage "S291" @default.
- W3100659219 startingPage "S277" @default.
- W3100659219 abstract "We present results from a 150ks Suzaku observation of the Seyfert 1.5 NGC3516 in 2005 October. The source was in a relatively highly absorbed state. Our best-fit model is consistent with the presence of a low-ionization absorber having a column density near 5|$times$|10|$^{22}$|cm|$^{-2}$| and covering most of the X-ray continuum source (covering fraction 96-100%). A high-ionization absorbing component, which yields a narrow absorption feature consistent with FeXXVIK, is confirmed. A relativistically broadened FeK|$alpha$| line was required in all fits, even after the complex absorption was taken into account; an additional partial-covering component is an inadequate substitute for the continuum curvature associated with the broad Fe line. A narrow FeK|$alpha$| emission line has a velocity width consistent with the Broad Line Region. The low-ionization absorber may be responsible for producing the narrow FeK|$alpha$| line, though a contribution from additional material out of the line of sight is possible. We include in our model soft band emission lines from He- and H-like ions of N, O, Ne, and Mg, consistent with photo-ionization, though a small contribution from collisionally-ionized emission is possible." @default.
- W3100659219 created "2020-11-23" @default.
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- W3100659219 date "2008-02-20" @default.
- W3100659219 modified "2023-10-16" @default.
- W3100659219 title "The Suzaku Observation of NGC3516: Complex Absorption and the Broad and Narrow FeK Lines" @default.
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- W3100659219 doi "https://doi.org/10.1093/pasj/60.sp1.s277" @default.
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