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   <subfield code="a">Cepheid kinematics and the Galactic warp</subfield>
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   <subfield code="a">The space velocities of 200 long-period (P&gt;5 days) classical Cepheids with known proper motions and line-of-sight velocities whose distances were estimated from the period-luminosity relation have been analyzed. The linear Ogorodnikov-Milne model has been applied, with the Galactic rotation having been excluded from the observed velocities in advance. Two significant gradients have been found in the Cepheid velocities, ∂W/∂Y = −2.1 ± 0.7 km s−1 kpc−1 and ∂V/∂Z = 27 ± 10 km s−1 kpc−1. In such a case, the angular velocity of solid-body rotation around the Galactic X axis directed to the Galactic center is −15 ± 5 km s−1 kpc−1.</subfield>
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