TYC 3134-790-1 , the SIMBAD biblio

TYC 3134-790-1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:00:25


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Title First 3 Authors
2011AJ....141...83P viz 15       D               1 1893 430 Kepler eclipsing binary stars. I. Catalog and principal characterization of 1879 eclipsing binaries in the first data release. PRSA A., BATALHA N., SLAWSON R.W., et al.
2011A&A...529A..89D viz 15       D               1 3298 98 Global stellar variability study in the field-of-view of the Kepler satellite. DEBOSSCHER J., BLOMME J., AERTS C., et al.
2011AJ....142..160S viz 15       D               1 2328 365 Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. SLAWSON R.W., PRSA A., WELSH W.F., et al.
2016ApJ...829...23D viz 16       D               1 4045 212 The Kepler catalog of stellar flares. DAVENPORT J.R.A.
2019MNRAS.485.2380M viz 16       D               1 14330 108 Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. MURPHY S.J., HEY D., VAN REETH T., et al.
2022ApJS..262...12K viz 60       D     X         2 792 7 A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit. KOBULNICKY H.A., MOLNAR L.A., COOK E.M., et al.
2023A&A...672A.176P viz 17       D               1 2155 2 Mass-ratio distribution of contact binary stars. PESTA M. and PEJCHA O.
2023A&A...672A.183A viz 17       D               1 15063 3 Astrophysical properties of 15062 Gaia DR3 gravity-mode pulsators Pulsation amplitudes, rotation, and spectral line broadening. AERTS C., MOLENBERGHS G. and DE RIDDER J.
2024A&A...685A..62I viz 18       D               1 2906 ~ Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al.
2025AJ....170..281C 93           X         2 30 ~ Observational Constraints on Close Binary Star Evolution. II. Extreme Mass Ratios. COOK E.M. and KOBULNICKY H.A.

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