Query= AG PEG GCVS Query forms

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

------------------------------------------------------------------------------------------------------------------------------------------------------------------

620061 |AG Peg *|215102.0+123732 |NC | 6.0 | 9.4 | |V | |1870 | | |WN6+M3III |09580 02510|

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

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

----------------------------------------------------------------------

620061 |AG Peg |215101.98 +123732.1 |+0.000 -0.003|2000.0 | |Hip

----------------------------------------------------------------------

_______________Cross-identifications:_______________

AG Peg = BD +11 4673 |

AG Peg = GSC 1130.00653 |

AG Peg = HD 207757 |

AG Peg = Hip 107848 |

AG Peg = IRAS 21486+1223 |

AG Peg = MWC 0379 |

AG Peg = SAO 107436 |

____________________________________________________ Reference to a chart or photograph:

02510. P.W.Merrill, Sky and Tel 18, N9, 490, 1959.

Reference to a study of the star:

09580. J.B.Hutchings, A.P.Cowley, R.O. Redman, ApJ 201, 404, 1975.

__________________________________________________________________

Remark:

    SB2 (Porb = 820d [09580]).

    Maximum of brightness was in 1870, then the very

    slow light decrease was observed that was superimposed

    since 1935 by periodical light oscillations with

    A = 0.4m V

    and P = Porb: Min = 2428250 + 827.d*E ( JD2428000-43000)

    [09587]. After JD2442300 the period probably has changed:

    Min = 2442370 + 760d*E [09587]. In 1962 - 1979 the range of

    brightness was 7.95m - 8.55m V; M - m = 0.50P.

    Light minima correspond to the epochs of inferior

    conjunction of M 3 III component. Spectrum var: Beq

    (1893 - 1919); since 1922 the spectrum is symbiotic one,

    the M star spectrum being more noticeable.

    Surrounded by a radio nebula with 1" half-power diameter.

----The End----