The Role of Complex Ionized Absorbers in the Soft X-Ray Spectra of Intermediate Polars

In magnetic cataclysmic variables (mCVs), X-ray radiation originates from a shock-heated, multi-temperature plasma in the post-shock region near white dwarf's surface. These X-rays are modified by complex distribution of absorbers pre-shock region. The presence photoionized lines and warm absorber features soft spectra these mCVs suggests that ionized. We developed ionized model zxipab, which is represented power-law flow. Using zxipab along with cooling flow reflection component, we broadband Chandra/High-Energy Transmission Grating (HETG) Nuclear Spectroscopic Telescope Array (NuSTAR) two intermediate polars (IPs): NY Lup V1223 Sgr. find this describes well many H- He-like emission medium-Z elements, arise collisionally excited plasma. However fails to account for some triplets points toward their origin. do not compelling evidence blackbody component excess seen residuals Chandra/HETG spectra, could be due uncertainties estimation interstellar absorption sources using data and/or fluxes accounted model. describe implications respect geometry IPs.