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EUV continuum of narrow-line Seyfert 1 galaxies

  • M. Dietrich (a1), D. M. Crenshaw (a1) and S. B. Kraemer (a2)

Abstract

We study the NLR emission line spectrum of 12 NLS1s to constrain the EUV – soft X-ray continuum SED using accurate photoionization modeling. We find that the NLR emission line ratios, which we measure for several NLS1 galaxies, can be reproduced within ±15% without a strong BBB component in the framework of a two-component model.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

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EUV continuum of narrow-line Seyfert 1 galaxies

  • M. Dietrich (a1), D. M. Crenshaw (a1) and S. B. Kraemer (a2)

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