Broadband X-ray spectrum of the intermediate polar V2400 Oph by the INTEGRAL and RXTE observatories. We reconstructed the spectrum of the source over
a wide (3-100 keV) energy
Broadband X-ray spectrum of intermediate polar V1223 Sgr of the spectrum in
a hard X-ray energy band (INTEGRAL/IBIS and RXTE/HEXTE) allowed us to disentangle contributions
The thickness of accretion α-disks: Theory and observations in these systems (up to h/
R ≈ 0.25, where h is the disk half-thickness and
R its radius), while standard α