SIMBAD references

2018RAA....18...20T - Research in Astron. and astroph., 18, 20-20 (2018/February-0)

Multi-color light curves and orbital period research of eclipsing binary V1073 Cyg.

TIAN X.-M., ZHU L.-Y., QIAN S.-B. and LI L.-J.

Abstract (from CDS):

New multi-color BVRcIc photometric observations are presented for the W UMa type eclipsing binary V1073 Cyg. The multi-color light curve analysis with the Wilson-Devinney procedure yielded the absolute parameters of this system, showing that V1073 Cyg is a shallow contact binary system with a fill-out factor f = 0.124(±0.011). We collected all available times of light minima spanning 119 yr, including CCD data to construct the O - C curve, and performed detailed O - C analysis. The O - C diagram shows that the period change is complex. A long-term continuous decrease and a cyclic variation exist. The period is decreasing at a rate of P = -1.04(±0.18) x 10–10 d cycle–1 and, with the period decrease, V1073 Cyg will evolve to the deep contact stage. The cyclic variation with a period of P3 = 82.7(±3.6) yr and an amplitude of A = 0.028(±0.002) d may be explained by magnetic activity of one or both components or the light travel time effect caused by a distant third companion with M3 (i' = 90°) = 0.511 M.

Abstract Copyright:

Journal keyword(s): stars: binaries: close - stars: binaries: eclipse - stars: binaries: individual: (V1073 Cyg)

Simbad objects: 14

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2020.09.25-01:16:00

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