Malacaria C, Bhargava Y, Coley JB, Ducci L, Pradhan P, Ballhausen R, Fuerst F, Islam N, Jaisawal GK, Jenke P, Kretschmar P, Kreykenbohm I, Pottschmidt K, Sokolova-Lapa E, Staubert R, Wilms J, Wilson-Hodge CA, Wolff MT (2022)
Publication Type: Journal article
Publication year: 2022
Book Volume: 927
Journal Issue: 2
Accreting X-ray pulsars undergo luminous X-ray outbursts during which the luminosity-dependent spectral and timing features of the neutron star's emission can be analyzed in detail, thus shedding light on the accretion regime at work. We took advantage of a monitoring campaign that was performed with NuSTAR, Swift/XRT, AstroSat and NICER to follow the Be/X-ray Binary 2S 1553-542 along one of its rare outbursts, and thus trace its spectral and timing evolution. We report the discovery of a luminosity-dependent cyclotron line energy for the first time in this source. The pulse profiles and pulsed fraction also show variability along the outburst, which is consistent with the interpretation that the source transitions from the subcritical to the supercritical accretion regime, separated by a critical luminosity of L (crit) approximate to 4 x 10(37) erg s(-1).
APA:
Malacaria, C., Bhargava, Y., Coley, J.B., Ducci, L., Pradhan, P., Ballhausen, R.,... Wolff, M.T. (2022). Accreting on the Edge: A Luminosity-dependent Cyclotron Line in the Be/X-Ray Binary 2S 1553-542 Accompanied by Accretion Regimes Transition. Astrophysical Journal, 927(2). https://doi.org/10.3847/1538-4357/ac524f
MLA:
Malacaria, C., et al. "Accreting on the Edge: A Luminosity-dependent Cyclotron Line in the Be/X-Ray Binary 2S 1553-542 Accompanied by Accretion Regimes Transition." Astrophysical Journal 927.2 (2022).
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