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| K2-138g , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST08:54:20 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2019A&A...631A..90L 
|
83 | C | 1 | 10 | 24 | Exoplanet characterisation in the longest known resonant chain: the K2-138 system seen by HARPS. | LOPEZ T.A., BARROS S.C.C., SANTERNE A., et al. | ||
| 2021AJ....161..219H | 894 | T | D | X C | 20 | 21 | 6 |
K2-138 g: Spitzer spots a sixth planet for the citizen science system. |
HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., CIARDI D.R., et al. |
|
2021ApJ...921...24S
|
17 | D | 1 | 328 | 1 | The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. | SCHLAUFMAN K.C. and HALPERN N.D. | ||
| 2022AJ....163..162M | 358 | D | X C | 8 | 11 | 4 | Confirming the 3:2 Resonance Chain of K2-138. | MacDONALD M.G., FEIL L., QUINN T., et al. | |
| 2022AJ....163..201G | 86 | C | 1 | 8 | 12 | Architectures of Compact Super-Earth Systems Shaped by Instabilities. | GOLDBERG M. and BATYGIN K. | ||
|
2022A&A...660A.102A
|
170 | X C | 3 | 37 | 4 | Water content trends in K2-138 and other low-mass multi-planetary systems. | ACUNA L., LOPEZ T.A., MOREL T., et al. | ||
| 2023ApJ...954...57C | 44 | A | D | 2 | 14 | ~ | A Six-planet Resonance Chain in K2-138? | CERIONI M. and BEAUGE C. | |
| 2023A&A...677A.160C | 131 | X F | 2 | 40 | ~ | Tidal interactions shape period ratios in planetary systems with three-body resonant chains. | CHARALAMBOUS C., TEYSSANDIER J. and LIBERT A.-S. | ||
| 2024ApJ...961..203M | 108 | D | F | 2 | 50 | ~ | Spin Dynamics of Planets in Resonant Chains. | MILLHOLLAND S.C., LARA T. and TOOMLAID J. | |
|
2024A&A...685A.143M
|
18 | D | 1 | 535 | ~ | Planets similar in size are often dissimilar in interior. | MAMONOVA E., SHAN Y., HATALOVA P., et al. | ||
|
2024A&A...687L...1L
|
18 | D | 2 | 140 | ~ | Resonant sub-Neptunes are puffier. | LELEU A., DELISLE J.-B., BURN R., et al. | ||
| 2026ApJ...996...12K | 50 | X | 1 | 19 | ~ | Higher-order Mean-motion Resonances Can Form in Type I Disk Migration. | KELLER F.M., DAI F. and XU W. |
