Multi-epoch XMM-Newton spectra of the two narrow-line Seyfert 1 (NLS1), Mrk 478 and EXO 1346.2+2645, are presented. The data were fitted with different models, including the relativistically blurred reflection model reflionx, which was found to give a good description of both spectra in all epochs. The two sources are reflection dominated with the illuminating continuum hidden from view. This can be explained in terms of either a corrugated disc or strong gravitational light bending effects. The emission from these two sources comes from a very small region (a few gravitational radii), very close to a rapidly spinning black hole. Spectral variability analysis shows that both sources have constant rms spectra, and constant hardness ratios in all epochs, in agreement with a single spectral component. The constancy spectrum between high and low states rules out alternative models such as partial covering. © 2008 RAS.
CITATION STYLE
Zoghbi, A., Fabian, A. C., & Gallo, L. C. (2008). Reflection-dominated X-ray spectra of narrow-line Seyfert 1 galaxies: Mrk 478 and EXO 1346.2+2645. Monthly Notices of the Royal Astronomical Society, 391(4), 2003–2008. https://doi.org/10.1111/j.1365-2966.2008.14078.x
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