TYC 3121-127-1 , the SIMBAD biblio

TYC 3121-127-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:29:10


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
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.
2013MNRAS.431.2240B viz 15       D               1 899 128 Activity in A-type stars. BALONA L.A.
2013A&A...557L..10N viz 15       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 15       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2015A&A...583A..65R viz 16       D               1 20938 134 Rotation, differential rotation, and gyrochronology of active Kepler stars. REINHOLD T. and GIZON L.
2018A&A...619A..98H 297       D     X C       7 70 27 The Kepler view of magnetic chemically peculiar stars. HUMMERICH S., MIKULASEK Z., PAUNZEN E., et al.
2019MNRAS.490.2112B viz 16       D               1 2864 ~ Evidence for spots on hot stars suggests major revision of stellar physics. BALONA L.A.
2022ApJS..259...63S viz 17       D               2 10269 2 Objective Separation between CP1 and CP2 Based on Feature Extraction with Machine Learning. SHANG L.-H., LUO A.-L., WANG L., et al.
2023A&A...672A.176P viz 17       D               1 2155 2 Mass-ratio distribution of contact binary stars. PESTA M. and PEJCHA O.
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.
2025MNRAS.538.3247B 299       D     X   F     6 37 ~ GALEX UV survey of magnetic chemically peculiar stars in the Kepler prime field. BERTONE E., HUMMERICH S., CHAVEZ M., et al.

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