Broadband study of X-Per using Suzaku observations

We present detailed broadband timing and spectral analysis of the persistent, low luminosity and slowly spinning pulsar 'X-per' using a Suzaku observation of the source. We have found for the first time, evidence for different intensity states with signatures of changes in the accretion geometry of the source. In addition, we confirm the presence of the cyclotron resonance at 30 keV which varies with the intensity states providing very crucial inputs on the accretion geometry.