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| TYC 3127-1423-1 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST12:00:59 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2012MNRAS.423.3420B | 92 | D | F | 2 | 89 | 71 | Kepler observations of flaring in A–F type stars. | BALONA L.A. | |
|
2013MNRAS.431.2240B |
15 | D | 2 | 899 | 128 | Activity in A-type stars. | BALONA L.A. | ||
|
2013A&A...560A...4R |
15 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
|
2015A&A...583A..65R |
16 | D | 2 | 20938 | 134 | Rotation, differential rotation, and gyrochronology of active Kepler stars. | REINHOLD T. and GIZON L. | ||
|
2016A&A...594A..39F |
16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
| 2017MNRAS.466.3060P | 532 | D | X C | 13 | 45 | 19 | Do A-type stars flare? | PEDERSEN M.G., ANTOCI V., KORHONEN H., et al. | |
|
2017MNRAS.467.1830B |
16 | D | 1 | 642 | 26 | Starspots on A stars. | BALONA L.A. | ||
|
2017ApJS..232...26V |
1 | 30 | 61 | Stellar flares observed in long-cadence data from the Kepler mission. | VAN DOORSSELAERE T., SHARIATI H. and DEBOSSCHER J. | ||||
|
2019MNRAS.485.2380M |
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. | ||
|
2019ApJS..241...29Y |
16 | D | 1 | 3420 | 70 | The flare catalog and the flare activity in the Kepler mission. | YANG H. and LIU J. | ||
|
2019MNRAS.490.2112B |
16 | D | 1 | 2864 | ~ | Evidence for spots on hot stars suggests major revision of stellar physics. | BALONA L.A. | ||
| 2020ApJ...905..110B | 16 | D | 2 | 53 | ~ | Flare properties of A-type stars in Kepler data. | BAI J.-Y. and ESAMDIN A. |