2020A&A...642A.196S

We summarize the results of a dedicated effort made between 2012 and 2019 to follow the evolution of the cyclotron line in Her X-1 through repeated NuSTAR observations. The previously observed nearly 20-year-long decay of the cyclotron line energy has ended in 2012: from then on, the pulse-phase-averaged flux-corrected cyclotron line energy has remained stable and constant at an average value of E_cyc=(37.44±0.07)keV (normalized to a flux level of 6.8 RXTE/ASM-cts/s). The flux dependence of E_cyc discovered in 2007 is now measured with high precision, giving a slope of (0.675±0.075) keV/(ASM-cts/s), corresponding to an increase of 6.5% of E_cyc for an increase in flux by a factor of two. We also find that all line parameters as well as the continuum parameters show a correlation with X-ray flux. While a correlation between E_cyc and X-ray flux (both positive and negative) is now known for several accreting binaries with various suggestions for the underlying physics, the phenomenon of a long-term decay has so far only been seen in Her X-1 and Vela X-1, with far less convincing explanations.