Photometric analysis of the eclipsing binary 2MASS 19090585+4911585

St Raetz; M. Vaňko; M. Mugrauer; T. O. B. Schmidt; T. Roell; T. Eisenbeiss; M. M. Hohle; A. Koeltzsch; Ch Ginski; C. Marka; M. Moualla; N. Tetzlaff; Ch Broeg; R. Neuhäuser

doi:10.1002/asna.200811206

Photometric analysis of the eclipsing binary 2MASS 19090585+4911585

St Raetz
, M. Vaňko
, M. Mugrauer
, T. O. B. Schmidt
, T. Roell
, T. Eisenbeiss
, M. M. Hohle
, A. Koeltzsch
, Ch Ginski
, C. Marka
, M. Moualla
, N. Tetzlaff
, Ch Broeg
, R. Neuhäuser

Physics

Research output: Contribution to a Journal (Peer & Non Peer) › Article › peer-review

Abstract

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 V RI light curves. The system is an overcontact binary of W UMa type with an orbital period of (0.288374 ± 0.000010) d.

Based on observations obtained with telescopes of the University Observatory Jena, which is operated by the Astrophysical Institute of the Friedrich-Schiller-University Jena....

Original language	English
Journal	Astronomische Nachrichten
DOIs	https://doi.org/10.1002/asna.200811206
Publication status	Published - May 2009

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title = "Photometric analysis of the eclipsing binary 2MASS 19090585+4911585",

abstract = "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 V RI light curves. The system is an overcontact binary of W UMa type with an orbital period of (0.288374 ± 0.000010) d. Based on observations obtained with telescopes of the University Observatory Jena, which is operated by the Astrophysical Institute of the Friedrich-Schiller-University Jena....",

author = "St Raetz and M. Va{\v n}ko and M. Mugrauer and Schmidt, \{T. O. B.\} and T. Roell and T. Eisenbeiss and Hohle, \{M. M.\} and A. Koeltzsch and Ch Ginski and C. Marka and M. Moualla and N. Tetzlaff and Ch Broeg and R. Neuh{\"a}user",

year = "2009",

month = may,

doi = "10.1002/asna.200811206",

language = "English",

journal = "Astronomische Nachrichten",

}

TY - JOUR

T1 - Photometric analysis of the eclipsing binary 2MASS 19090585+4911585

AU - Raetz, St

AU - Vaňko, M.

AU - Mugrauer, M.

AU - Schmidt, T. O. B.

AU - Roell, T.

AU - Eisenbeiss, T.

AU - Hohle, M. M.

AU - Koeltzsch, A.

AU - Ginski, Ch

AU - Marka, C.

AU - Moualla, M.

AU - Tetzlaff, N.

AU - Broeg, Ch

AU - Neuhäuser, R.

PY - 2009/5

Y1 - 2009/5

N2 - 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 V RI light curves. The system is an overcontact binary of W UMa type with an orbital period of (0.288374 ± 0.000010) d. Based on observations obtained with telescopes of the University Observatory Jena, which is operated by the Astrophysical Institute of the Friedrich-Schiller-University Jena....

AB - 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 V RI light curves. The system is an overcontact binary of W UMa type with an orbital period of (0.288374 ± 0.000010) d. Based on observations obtained with telescopes of the University Observatory Jena, which is operated by the Astrophysical Institute of the Friedrich-Schiller-University Jena....

U2 - 10.1002/asna.200811206

DO - 10.1002/asna.200811206

M3 - Article

JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

ER -

Photometric analysis of the eclipsing binary 2MASS 19090585+4911585

Abstract

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