Kühnel M, Müller S, Kreykenbohm I, Fuerst F, Pottschmidt K, Rothschild RE, Caballero I, Grinberg V, Schoenherr G, Shrader C, Klochkov D, Staubert R, Ferrigno C, Torrejon JM, Martinez-Nunez S, Wilms J (2014)
Publication Status: Published
Publication Type: Conference contribution
Publication year: 2014
Book Volume: 64
Article Number: UNSP 06003
DOI: 10.1051/epjconf/20136406003
In a former publication, we have analyzed the transient neutron star X-ray binary GRO J1008-57 using all available RXTE-, Swift-, and Suzaku-data. As we have found, the source's spectral components, i.e., a power-law with high exponential cutoff and a black-body, are strongly correlated with the hard X-ray flux (15-50 keV). We update the analytical description of these dependence, including a change in the photon index behaviour from a flat to a logarithmic function. The flux, where the change occurs, is consistent with the onset of the black-body emission. Thus, a change of the accretion state always occurs in GRO J1008-57 at a particular flux level.
APA:
Kühnel, M., Müller, S., Kreykenbohm, I., Fuerst, F., Pottschmidt, K., Rothschild, R.E.,... Wilms, J. (2014). Luminosity dependent accretion state change in GRO J1008-57.
MLA:
Kühnel, Matthias, et al. "Luminosity dependent accretion state change in GRO J1008-57." 2014.
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