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Active Galactic Nuclei with High-Resolution X-Ray Spectroscopy

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High-Resolution X-ray Spectroscopy

Part of the book series: Springer Series in Astrophysics and Cosmology ((SSAC))

Abstract

The imminent launch of XRISM will usher in an era of high-resolution X-ray spectroscopy. For active galactic nuclei (AGN) this is an exciting epoch that is full of massive potential for uncovering the ins and outs of supermassive black hole accretion. In this work, we review AGN research topics that are certain to advance in the coming years with XRISM and prognosticate the possibilities with Athena and Arcus. Specifically, our discussion focuses on: (i) the relatively slow moving ionised winds known as warm absorbers and obscurers; (ii) the iron emitting from different regions of the inner and outer disc, broad line region, and torus; and (iii) the ultrafast outflows that may be the key to understanding AGN feedback.

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Notes

  1. 1.

    The Eddington luminosity, \(L_{Edd}=1.26\times 10^{38} M_{BH}/M_{\odot }\mathrm erg~s^{-1}\), is the maximum luminosity a system can have such that the gravitational infall of ionised hydrogen gas is exactly balanced by the outward radiation pressure.

  2. 2.

    In this section, all illustrations are produced using the SPEX package [107].

  3. 3.

    The reflection fraction is the ratio of reflected flux to primary flux.

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Acknowledgements

The authors would like to thank Margaret Buhariwalla, Susmita Chackravorty, Keigo Fukumura, Adam Gonzalez, Jelle Kaastra, Tim Kallman, Gabriele Matzeu, Missagh Mehdipour, Daniel Proga, John Raymond, Daniele Rogantini for discussion, data, code, and help with figures.

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  1. Department of Astronomy and Physics, Saint Mary’s University, 923 Robie Street, Halifax, NS B3H 3C3, Canada

    Luigi C. Gallo

  2. Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI, 48109, USA

    Jon M. Miller

  3. SRON Netherlands Institute for Space Research, Niels Bohrweg 4, 2333CA, Leiden, The Netherlands

    Elisa Costantini

  4. Anton Pannekoek Astronomical Institute, University of Amsterdam, Postbus 94249, NL-1090 GE, Amsterdam, The Netherlands

    Elisa Costantini

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    Jiachen Jiang

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Gallo, L.C., Miller, J.M., Costantini, E. (2023). Active Galactic Nuclei with High-Resolution X-Ray Spectroscopy. In: Bambi, C., Jiang, J. (eds) High-Resolution X-ray Spectroscopy. Springer Series in Astrophysics and Cosmology. Springer, Singapore. https://doi.org/10.1007/978-981-99-4409-5_9

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