Detection of a fully resolved Compton shoulder of the iron K alpha line in the Chandra X-ray spectrum of GX 301-2

We report the detection of a fully resolved, Compton-scattered emission line in the X-ray spectrum of the massive binary GX 301-2 obtained with the High Energy Transmission Grating Spectrometer on board the Chandra X-Ray Observatory. The iron Kalpha fluorescence line complex observed in this system consists of an intense narrow component centered at an energy of E = 6.40 keV and a redward shoulder that extends down to similar to6.24 keV, which corresponds to an energy shift of a Compton backscattered iron Kalpha photon. From detailed Monte Carlo simulations and comparisons with the observed spectra, we are able to directly constrain the physical properties of the scattering medium, including the electron temperature and column density, as well as an estimate for the metal abundance.