BD-19 4173b , the SIMBAD biblio

BD-19 4173b , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST06:53:21


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Title First 3 Authors
2019MNRAS.484.3522H 709       D     X C F     16 6 17 K2-290: a warm Jupiter and a mini-Neptune in a triple-star system. HJORTH M., JUSTESEN A.B., HIRANO T., et al.
2019A&A...630A.135U viz 16       D               1 501 16 Beyond the exoplanet mass-radius relation. ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., et al.
2022ApJ...925L...5B 128           X         3 7 4 The Chaotic History of the Retrograde Multi-planet System in K2-290A Driven by Distant Stars. BEST S. and PETROVICH C.
2022PASP..134h2001A viz 60       D     X         2 366 39 Stellar Obliquities in Exoplanetary Systems. ALBRECHT S.H., DAWSON R.I. and WINN J.N.
2022ApJS..263...33C 17       D               1 85 2 An Early Catalog of Planet-hosting Multiple-star Systems of Order Three and Higher. CUNTZ M., LUKE G.E., MILLARD M.J., et al.
2023ApJ...944L..41F viz 131           X         3 19 2 NEID Reveals That the Young Warm Neptune TOI-2076 b Has a Low Obliquity. FRAZIER R.C., STEFANSSON G., MAHADEVAN S., et al.
2023A&A...674A.120A 17       D               1 189 1 DREAM II. The spin-orbit angle distribution of close-in exoplanets under the lens of tides. ATTIA O., BOURRIER V., DELISLE J.-B., et al.
2023MNRAS.524.1113S 17       D               1 85 ~ TESS spots a mini- interior to a hot saturn in the TOI-2000 system. SHA L., VANDERBURG A.M., HUANG C.X., et al.
2024MNRAS.528..270K 63       D     X         2 22 ~ The flipped orbit of KELT-19Ab inferred from the symmetric TESS transit light curves. KAWAI Y., NARITA N., FUKUI A., et al.
2024AJ....167..126R 90             C       1 141 ~ The Orbital Geometries and Stellar Obliquities of Exoplanet-hosting Multistar Systems. RICE M., GERBIG K. and VANDERBURG A.
2024A&A...685A.143M viz 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 viz 90           X         2 140 ~ Resonant sub-Neptunes are puffier. LELEU A., DELISLE J.-B., BURN R., et al.
2024A&A...690A.379K 90           X         2 72 ~ Obliquities of exoplanet host stars Nineteen new and updated measurements, and trends in the sample of 205 measurements. KNUDSTRUP E., ALBRECHT S.H., WINN J.N., et al.
2024AJ....168..194T 45           X         1 6 ~ The ∼50 Myr Old TOI-942c is Likely on an Aligned, Coplanar Orbit and Losing Mass. TENG H.-Y., DAI F., HOWARD A.W., et al.
2024AJ....168..196L viz 45           X         1 27 ~ The HD 191939 Exoplanet System is Well Aligned and Flat. LUBIN J., PETIGURA E.A., VAN ZANDT J., et al.
2024ApJ...974..304L 45           X         1 10 ~ Polar Neptunes Are Stable to Tides. LOUDEN E.M. and MILLHOLLAND S.C.
2025ApJ...988..247S 112       D     X         3 31 ~ Tidal Inflation is Stronger for Misaligned Neptune-sized Planets Than Aligned Ones. SETHI R. and MILLHOLLAND S.C.
2025AJ....170..175Z 140           X         3 11 ~ TOI-880 is an Aligned, Coplanar, Multiplanet System. ZHANG E.Y., TENG H.-Y., DAI F., et al.
2025AJ....170..182P 19       D               1 58 ~ An Aligned Sub-Neptune Revealed with MAROON-X and a Tendency Toward Alignment for Small Planets. POLANSKI A.S., CROSSFIELD I.J.M., SEIFAHRT A., et al.
2025ApJS..281...61L 19       D               1 643 ~ Stellar Characterization, Magnesium Abundances, and Chromospheric Activity Analysis of Stars with Confirmed Exoplanets from the K2 Mission. LOAIZA-TACURI V., SOUTO D., QUISPE-HUAYNASI F., et al.
2026A&A...705A.142R viz 20       D               1 55 ~ True spin-orbit obliquity distribution: Data-driven confirmation of no clustering of misaligned planets. ROSSI A.M., RAINER M., BORSA F., et al.
2026ApJ...997..327B 100           X         2 10 ~ Warm Jupiter Tidal Migration Can Spare Inner Planets; Hot Jupiter Tidal Migration May Not. BECKER J.
2026ApJ...999...36L 1300     A D     X C       26 17 ~ Atmospheric Circulation of High-obliquity Mini-Neptunes. LAI Y., TAN X. and SU Y.

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