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   <subfield code="a">Orientation parameters of the Cepheid system in the Galaxy</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[V. Bobylev]</subfield>
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   <subfield code="a">Based on the distribution of long-period Cepheids, we have redetermined the orientation parameters of their principal plane in the Galaxy. Based on 299 Cepheids with heliocentric distances r &lt; 20 kpc and pulsation periods P ≥ 5d, we have found the directions of the three principal axes of the position ellipsoid: L 1 = 281.0° ± 0.1°, B 1 = −1.9° ± 0.1°; L 2 = 11.0° ± 0.7°, B 2 = 0.2° ± 0.1°; and L 3 = 275.9° ± 0.7°, B 3 = 88.1° ± 0.1°. Thus, the line of nodes l Ω = L 3 + 90° = 5.9° is very close to the direction to the Galactic center; the Cepheid symmetry plane is inclined to the Galactic plane approximately by −2° in the direction of the first axis (L 1). The direction of the line of nodes found from old Cepheids (P &lt;5d) differs significantly and is l Ω = 298°. The elevation of the Sun above the Galactic plane has been estimated from 365 closer stars (r &lt; 4 kpc) without any constraint on the pulsation period to be h ⊙ = 23 ± 5 kpc.</subfield>
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