Query= V389 CYG GCVS Query forms

NNo GCVS J2000.0 Type Max Min I Min II Epoch(JD24..) Year Period M-m/D Spectrum References Other design.

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310389 |V0389 Cyg *|210838.9+301220 |* | 5.55 | 5.71 | |V | | | | |B9Vp(Si) |01256 01182|

------------------------------------------------------------------------------------------------------------------------------------------------------------------ ______________The positional information: ___________________________

NNo GCVS J2000.0 p.m.(as/yr) Epoch Ident.

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310389 |V0389 Cyg |210838.89 +301220.3 |+0.025 -0.021|2000.0 | |Hip

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_______________Cross-identifications:_______________

V0389 Cyg = ADS 14682 |A

V0389 Cyg = BD +29 4324 |

V0389 Cyg = BS 08094 |

V0389 Cyg = GSC 2701.03919 |

V0389 Cyg = HD 201433 |

V0389 Cyg = Hip 104371 |

V0389 Cyg = SAO 070968 |

____________________________________________________ Reference to a chart or photograph:

01182. H.Schneller, Sterne 17, 87, 1937.

Reference to a study of the star:

01256. P.Guthnick, Sterne 22, 129, 1942.

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Remark:

    VB A (B 8.0m, 3.4", 305deg, 1980). SB (P = 3.313168d);

    Turns around the invisible third companion with

    P = 154.09d. According to [01256] the light varies with

    two alternate periods P1 and P2. The first oscillation

    (P1) with A = 0.19m satisfies the elements: Max =

    2423298.460 + 1.12912d*E, the second (P2) with A =

    0.05m - the elements: Max = 2429162.080 + 1.19328d*E.

    each of them continues for 1 - 3 weeks. At the transition

    from one oscillation to the other irregular light

    variations are sometimes observed or almost constant

    brightness. At the renewal of each oscillation its phase

    remains unchanged, experiencing no shift. According

    to [08909] in 1975 - 1977 periodicity was not observed.

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