LP 413-32 B , the SIMBAD biblio

LP 413-32 B , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST18:17:47


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Title First 3 Authors
2019AJ....157...40F 81           X         2 16 7 K2-288Bb: a small temperate planet in a low-mass binary system discovered by citizen scientists. FEINSTEIN A.D., SCHLIEDER J.E., LIVINGSTON J.H., et al.
2019AJ....158...87D viz 41           X         1 179 ~ Characterizing K2 candidate planetary systems orbiting low-mass stars. IV. Updated properties for 86 cool dwarfs observed during Campaigns 1-17. DRESSING C.D., HARDEGREE-ULLMAN K., SCHLIEDER J.E., et al.
2019ApJ...887..261M viz 16       D               3 329 29 Exomoons in the habitable zones of M dwarfs. MARTINEZ-RODRIGUEZ H., CABALLERO J.A., CIFUENTES C., et al.
2020ApJ...890...23L viz 16       D               1 4936 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020AJ....159...80Q 41           X         1 48 ~ Orbital stability of circumstellar planets in binary systems. QUARLES B., LI G., KOSTOV V., et al.
2023MNRAS.520.5283G 87           X         2 91 6 The TIME Table: rotation and ages of cool exoplanet host stars. GAIDOS E., CLAYTOR Z., DUNGEE R., et al.
2023MNRAS.525.5168M 17       D               1 68 ~ Impact of M-dwarf stellar wind and photoevaporation on the atmospheric evolution of small planets. MODI A., ESTRELA R. and VALIO A.
2024A&A...689A.302G viz 108       D     X         3 1270 ~ Multiplicity of stars with planets in the solar neighbourhood. GONZALEZ-PAYO J., CABALLERO J.A., GORGAS J., et al.
2024A&A...691A..53S viz 18       D               2 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2025AJ....169...13P 112       D         F     2 94 ~ The 10 pc Neighborhood of Habitable Zone Exoplanetary Systems: Threat Assessment from Stellar Encounters and Supernovae. PYNE T., BANYAL R.K., SWASTIK C., et al.

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