NNo GCVS J2000.0 Type Max Min I Min II Epoch Year Period M-m/D Spectrum References Other desig. p.m.(as/yr) Epoch Ident. New type GCVS -------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- 080238 |IU Aur *|052752.40 +344658.3 |EB | 8.19 | 8.89 | 8.74 |V |38448.4068 | | 1.81147435 | |B0p+B1Vp |N0175 HIP | |+0.001 +0.000|2000.0 | |Hip |EC |IU Aur | -------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------------- _______________Cross-identifications:_______________ IU Aur = BD +34 1051 | IU Aur = GSC 2411.01941 | IU Aur = HD 035652 | IU Aur = Hip 025565 | IU Aur = SAO 058059 | ____________________________________________________ Reference to a chart or photograph:HIP The Hipparcos and Tycho Catalogues (European Space Agency, 1997), ESA SP-1200 (CDS Cat. I/239) {1997ESASP1200.....E}
Reference to a study of the star:
N0175. P. Mayer, BAC 38, No. 1, 58, 1987.__________________________________________________________________
Remark: A well-documented light-time effect (P = 294.3d, the semi-amplitude of the O-C residuals is 0.0059d) because of a third body on an eccentric orbit. Precession causes changes of the brightness amplitude: the amplitude of the MinI was observed to vary between 0.46m and 0.70m and that of MinII, between 0.37m and 0.55m. The depths of minima reached their maximum values about JD 2445800 and began to decrease [N0176].
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