Cyclotron line energy in Hercules X-1: Stable after the decay

Staubert R, Ducci L, Ji L, Fürst F, Wilms J, Rothschild RE, Pottschmidt K, Brumback M, Harrison F (2020)


Publication Type: Journal article

Publication year: 2020

Journal

Book Volume: 642

Article Number: A196

DOI: 10.1051/0004-6361/202038855

Abstract

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 Ecyc = (37.44 ± 0.07) keV (normalized to a flux level of 6.8 RXTE/ASM-cts s-1). The flux dependence of Ecyc discovered in 2007 is now measured with high precision, giving a slope of (0.675 ± 0.075) keV/(ASM-cts s-1), corresponding to an increase of 6.5% of Ecyc 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 Ecyc 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.

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APA:

Staubert, R., Ducci, L., Ji, L., Fürst, F., Wilms, J., Rothschild, R.E.,... Harrison, F. (2020). Cyclotron line energy in Hercules X-1: Stable after the decay. Astronomy & Astrophysics, 642. https://doi.org/10.1051/0004-6361/202038855

MLA:

Staubert, R., et al. "Cyclotron line energy in Hercules X-1: Stable after the decay." Astronomy & Astrophysics 642 (2020).

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