Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

XRISM/Resolve Spectroscopy of the Central Engine in the Seyfert-1 AGN Mrk 279

  • Authors: Jon M. Miller, Xin Xiang, Doyee Byun, 도의 변, Ehud Behar, Laura Brenneman, Edward Cackett, Elisa Costantini, Luigi Gallo, Keith Horne, Elias Kammoun, Chen Li, Abderahmen Zoghbi

Jon M. Miller et al 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure 5.

A comparison of the inner radii measured for Fe Kα line components in a subset of XRISM spectra of local AGN. All of the radii are based on blurred “mytorus” modeling of Resolve spectra; please see the text for details. With several important caveats, this plot suggests that Resolve data are able to separate line emission from the inner disk, BLR, and torus and capable of tracing trends with Eddington fraction.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse