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Catalog Service:
Minimum times of 7 eclipsing systems

Short name: J/AJ/147/130
IVOA Identifier: ivo://CDS.VizieR/J/AJ/147/130
DOI (Digital Object Identifier): 10.26093/cds/vizier.51470130
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/147/130
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2014 Sep 24 14:57:56Z
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Description


The minimum timings of eclipsing binaries V418 Aql, SU Boo, RV CVn, CR Cas, GV Cyg, V432 Per, and BD+42 2782 were collected and analyzed. Their long-term behavior was studied via period analysis, revealing a periodic term in eclipse times. We derived 576 new times of minimum. Hence, to describe the periodic variation, a third-body hypothesis was proposed and the resulting orbital periods are as follows: 70, 7.4, 53, 37, 27, 53, and 18 yr, respectively. For the system V432 Per an additional 9.5 yr variation was also found. The predicted minimum masses of these distant bodies were calculated and their detectability discussed. The light curves of SU Boo and RV CVn were analyzed using the PHOEBE program, resulting in physical parameters of the components. New variable stars in the field of V418 Aql were discovered.

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