GCVS Query forms

Query= EPS AUR 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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089005 |eps Aur *|050158.1+434924 |EA | 2.92 | 3.88 | |V |45513. | | 9884. |08 |A8Iab: |00001 HIP |

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

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

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089005 |eps Aur |050158.13 +434923.9 |+0.000 -0.002|2000.0 | |Hip

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_______________Cross-identifications:_______________

eps Aur = ADS 03605 |A

eps Aur = BAY Aur eps |

eps Aur = BD +43 1166 |

eps Aur = BS 01605 |

eps Aur = CRL 0670S |

eps Aur = FLM Aur 007 |

eps Aur = GSC 2907.01275 |

eps Aur = HD 031964 |

eps Aur = Hip 023416 |

eps Aur = IRAS 04583+4345 |

eps Aur = IRC +40109 |

eps Aur = SAO 039955 |

____________________________________________________ Reference to a chart or photograph:

HIP The Hipparcos and Tycho Catalogues (European Space Agency, 1997), ESA SP-1200 (CDS Cat. I/239).

Reference to a study of the star:

00001. GCVS compilers.

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Remark:

    d =  0.04 P.

    VB A (B 14.0m, 30", 225deg, 2008; C 11.3m, 43", 276deg, 2008;

    D 12.0m, 45", 316deg, 2008). Probably eclipses are caused by

    a gas and dust disk. Besides eclipses, quasi-periodic brightness

    variations with an amplitude of several tenths of a magnitude

    and a cycle of 105 - 120 days (e.g., [N0204]). More rapid

    variations were also reported.

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