V* V637 Peg , the SIMBAD biblio

V* V637 Peg , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:26:54


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Title First 3 Authors
2006AJ....131..621G viz 15       D               1 1033 125 A catalog of 1022 bright contact binary stars. GETTEL S.J., GESKE M.T. and McKAY T.A.
2009AJ....138..466H viz 15       D               1 4127 116 Automated variable star classification using the Northern Sky Variability Survey. HOFFMAN D.I., HARRISON T.E. and McNAMARA B.J.
2014ApJS..213....9D viz 15       D               1 46794 385 The Catalina surveys periodic variable star catalog. DRAKE A.J., GRAHAM M.J., DJORGOVSKI S.G., et al.
2018AJ....156..241H viz 16       D               1 311106 199 A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). HEINZE A.N., TONRY J.L., DENNEAU L., et al.
2017RMxAA..53..235K viz 659     A     X C       16 34 6 Observations and light curve solutions of six deep-contact W UMA binaries. KJURKCHIEVA D.P., POPOV V.A., VASILEVA D.L., et al.
2019AJ....158..186K viz 16       D               1 48 ~ Global parameters of 12 totally eclipsing W UMa stars. KJURKCHIEVA D.P., POPOV V.A. and PETROV N.I.
2020RAA....20..163Q viz 16       D               4 8835 46 Contact binaries at different evolutionary stages. QIAN S.-B., ZHU L.-Y., LIU L., et al.
2021ApJS..254...10L viz 17       D               1 694 37 Statistics of 700 individually studied W UMa stars. LATKOVIC O., CEKI A. and LAZAREVIC S.
2023A&A...674A..16M viz 17       D               1 2184478 19 Gaia Data Release 3 The first Gaia catalogue of eclipsing-binary candidates. MOWLAVI N., HOLL B., LECOEUR-TAIBI I., et al.
2024ApJS..273...31W viz 18       D               1 5142 ~ A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey. WANG J., DING X., LI J., et al.
2025PASP..137l4202P 578       D     X         13 24 ~ BSN. V. The First Detailed Light Curve Modeling of Eight Totally Eclipsing Contact Binary Stars Using Ground-based and TESS Observations. PORO A., MICHEL R., TAMAYO F.J., et al.

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