2MASS J19230559+3848519 , the SIMBAD biblio

2MASS J19230559+3848519 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:53:27


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Title First 3 Authors
2013A&A...556A..52T viz 16       D               1 265 46 Detection of a large sample of γ Doradus stars from Kepler space photometry and high-resolution ground-based spectroscopy. TKACHENKO A., AERTS C., YAKUSHECHKIN A., et al.
2013A&A...557L..10N viz 16       D               1 12151 189 Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. NIELSEN M.B., GIZON L., SCHUNKER H., et al.
2013A&A...560A...4R viz 16       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2014A&A...568A..34B 315         O X C       7 19 14 Wavelets: a powerful tool for studying rotation, activity, and pulsation in Kepler and CoRoT stellar light curves. BRAVO J.P., ROQUE S., ESTRELA R., et al.
2015ApJS..218...27V 16       D               3 73 114 Gravity-mode period spacings as a seismic diagnostic for a sample of γ Doradus stars from Kepler space photometry and high-resolution ground-based spectroscopy. VAN REETH T., TKACHENKO A., AERTS C., et al.
2016ApJ...829...23D viz 16       D               1 4044 212 The Kepler catalog of stellar flares. DAVENPORT J.R.A.
2019MNRAS.485.2380M viz 17       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.
2019MNRAS.490.2112B viz 17       D               1 2864 ~ Evidence for spots on hot stars suggests major revision of stellar physics. BALONA L.A.
2020MNRAS.491.3586L viz 17       D               1 609 75 Gravity-mode period spacings and near-core rotation rates of 611 γ Doradus stars with Kepler. LI G., VAN REETH T., BEDDING T.R., et al.
2021A&A...650A.151G 17       D               4 131 14 A homogeneous spectroscopic analysis of a Kepler legacy sample of dwarfs for gravity-mode asteroseismology. GEBRUERS S., STRAUMIT I., TKACHENKO A., et al.

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