Reflection spectra in the non-relativistic case and a neutral accretion disk for three models; the inclination angle increases from left to right. The incident power-law spectrum is the black curve; the xillver, pexrav, and a Monte Carlo simulation are shown as red, blue, and yellow curves, respectively. We use wilm abundances (Wilms et al. 2000), except for xillver for which we use grsa abundances (Grevesse & Sauval 1998). The highlighted area shows the energy band of the Compton hump, which is used to calculate the reflection strength.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.