1999A&A...346..125H

The Super Soft Source RX J0925.7-4758 (RX J0925 hereafter) was observed by BeppoSAX LECS and MECS on January 25-26 1997. The source was clearly detected by the LECS but only marginally detected by the MECS. We apply detailed Non-Local Thermodynamic Equilibrium (Non-LTE) models including metal line opacities to the observed LECS spectrum. We test whether the X-ray spectrum of RX J0925 is consistent with that of a white dwarf and put constraints upon the effective temperature and surface gravity by considering the presence or absence of spectral features such as absorption edges and line blends in the models and the observed spectrum. We find that models with effective temperatures above ∼10⁶K or below ∼7.5x10⁵K can be excluded. If we assume a single model component for RX J0925 we observe a significant discrepancy between the model and the data above the Neix edge energy at 1.19keV. This is consistent with earlier observations with ROSAT and ASCA. The only way to account for the emission above ∼1.2keV is by introducing a second spectral (plasma) component. This plasma component may be explained by a shocked wind originating from the compact object or from the irradiated companion star. If we assume logg=9 then the derived luminosity is consistent with that of a nuclear burning white dwarf at a distance of ∼4kpc.