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arXiv · 1909.13242

A correlation between [O III] line property and X-ray spectral complexity in narrow-line Seyfert 1 galaxies?

S. Chen·G. La Mura·M. Berton·L. Foschini·E. Congiu·F. Di Mille·S. Ciroi·E. Bottacini·J. H. Fan·A. Vietri
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Abstract

We present a detailed study of 11 narrow-line Seyfert 1 galaxies (NLS1s) from the Six-degree Field Galaxy Survey (6dFGS) that both have optical and X-ray spectroscopic observations. There are five complex NLS1s (C-NLS1s) and six simple NLS1s (S-NLS1s). We propose a possible correlation between [O III] line asymmetry and X-ray complexity. The outflow or wind from the inner accretion disk is commonly present in NLS1s and mostly directed along the system axis. In C-NLS1s only weak wind effects are measured, the X-ray spectral complexity might be caused by the presence of ionized material in the wind. On the contrary, the wind in S-NLS1s is fast, the ionized material could be swept by such a strong wind, thus the complex feature is missing which results in a simple X-ray spectrum. Furthermore, this outflow scenario seems to be an inclination effect. Since the speed of the wind is higher in a small inclination while lower in a large inclination, S-NLS1s might be sources viewed at small angles while C-NLS1s might be sources viewed at large angles.

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S. Chen, G. La Mura, M. Berton, L. Foschini, E. Congiu, F. Di Mille, S. Ciroi, E. Bottacini, J. H. Fan, A. Vietri. 2019-09-29. A correlation between [O III] line property and X-ray spectral complexity in narrow-line Seyfert 1 galaxies?. https://arxiv.org/abs/1909.13242

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