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 veryslow light decrease was observed that was superimposedsince 1935 by periodical light oscillations withA = 0.4m Vand 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 ofbrightness was 7.95m - 8.55m V; M - m = 0.50P.Light minima correspond to the epochs of inferiorconjunction 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----