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We present new results on X-ray properties of radio loud broad absorptionline (BAL) quasars and focus on broad-band spectral properties of a highionization BAL (HiBAL) compact steep spectrum (CSS) radio-loud quasar 1045+352.This HiBAL quasar has a very complex radio morphology indicating either stronginteractions between a radio jet and the surrounding interstellar medium or apossible re-start of the jet activity. We detected 1045+352 quasar in a short 5ksec Chandra ACIS-S observation. We applied theoretical models to explainspectral energy distribution (SED) of 1045+352 and argue that non-thermal,inverse-Compton emission from the innermost parts of the radio jet can accountfor a large fraction of the observed X-ray emission. In our analysis we alsoconsider a scenario in which the observed X-ray emission from radio-loud BALquasars can be a sum of inverse-Compton jet X-ray emission and optically thincorona X-ray emission. We compiled a sample of radio-loud BAL quasars that wereobserved in X-rays to date and report no correlation between their X-ray andradio luminosity. However, the radio-loud BAL quasars show a large range ofX-ray luminosities and absorption columns. This is consistent with the resultsobtained earlier for radio-quiet BAL quasars and may indicate an orientationeffect in BAL quasars or more complex dependence between X-ray emission, radioemission and an orientation based on the radio morphology.

X-rays from a radio-loud compact BAL Quasar 1045+352 and the nature of outflows in radio-loud BAL Quasars