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The Long Stare at Hercules X-1. I. Emission Lines from the Outer Disk, the Magnetosphere Boundary, and the Accretion Curtain

  • Authors: P. Kosec, E. Kara, A. C. Fabian, F. Fürst, C. Pinto, I. Psaradaki, C. S. Reynolds, D. Rogantini, D. J. Walton, R. Ballhausen, C. Canizares, S. Dyda, R. Staubert, J. Wilms

P. Kosec et al 2022 The Astrophysical Journal 936 .

  • Provider: AAS Journals

Caption: Figure 8.

The 1D velocity (left y-axes) and FWHM widths (right y-axes) of the Fe XXV (top panel) and O VIII/N VII (bottom panel) lines vs. the super-orbital phase. The right y-axis on the bottom panel only contains the FWHM width of the O VIII line. The observations with XMM-Newton during the 2020 campaign are shown in black, archival XMM-Newton observations are shown in blue, and Chandra observations are shown in red.

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