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Paper detail

Photometric analysis of the eclipsing binary 2MASS 19090585+4911585

We report on observations of the eclipsing binary 2MASS 19090585+4911585 with the 25 cm auxiliary telescope of the University Observatory Jena. We show that a nearby brighter star (2MASS 19090783+4912085) was previously misclassified as the eclipsing binary and find 2MASS 19090585+4911585 to be the true source of variation. We present photometric analysis of VRI light curves. The system is an overcontact binary of W UMa type with an orbital period of (0.288374 +/- 0.000010) d.

preprint2009arXivOpen access
St. RaetzM. VankoM. MugrauerT. O. B. SchmidtT. RoellT. EisenbeissM. M. HohleA. KoeltzschCh. GinskiC. MarkaM. MouallaN. TetzlaffCh. BroegR. Neuhäuser
astro-ph.SR
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St. RaetzM. VankoM. MugrauerT. O. B. SchmidtT. RoellT. EisenbeissM. M. HohleA. KoeltzschCh. GinskiC. MarkaM. MouallaN. TetzlaffCh. BroegR. Neuhäuser

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