[QWL2012] Pr0211b , the SIMBAD biblio

[QWL2012] Pr0211b , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.01.27CET19:24:19


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Title First 3 Authors
2012ApJ...756L..33Q viz 65     A     X         2 11 67 Two "b"s in the Beehive: the discovery of the first hot Jupiters in an open cluster. QUINN S.N., WHITE R.J., LATHAM D.W., et al.
2013A&A...552A.119S viz 16       D               1 1487 42 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2013ApJ...772..142L 39           X         1 15 10 Configurations of bounded and free-floating planets in very young open clusters. LIU H.-G., ZHANG H. and ZHOU J.-L.
2016A&A...588A.118M viz 2 14 35 The GAPS programme with HARPS-N at TNG. XI. Pr 0211 in M 44: the first multi-planet system in an open cluster. MALAVOLTA L., NASCIMBENI V., PIOTTO G., et al.
2017MNRAS.470.4337C 16       D               1 27 10 Stability of multiplanetary systems in star clusters. CAI M.X., KOUWENHOVEN M.B.N., PORTEGIES ZWART S.F., et al.
2017ApJ...848...20W 16       D               1 27 2 Forming different planetary architectures. I. The formation efficiency of hot Jupiters from high-eccentricity mechanisms. WANG Y., ZHOU J.-L., HUI-GEN L., et al.
2018AJ....155...10C 42           X         1 30 16 K2-136: a binary system in the Hyades Cluster hosting a Neptune-sized planet. CIARDI D.R., CROSSFIELD I.J.M., FEINSTEIN A.D., et al.
2018A&A...610A..33P 100       D     X         3 18 1 Did a stellar fly-by shape the planetary system around Pr 0211 in the cluster M44? PFALZNER S., BHANDARE A. and VINCKE K.
2018AJ....155..173C viz 17       D               1 62 5 K2-231 b: a sub-Neptune exoplanet transiting a solar twin in Ruprecht 147. CURTIS J.L., VANDERBURG A., TORRES G., et al.
2018MNRAS.475.3090Y viz 17       D               1 483 ~ Forecasting the detectability of known radial velocity planets with the upcoming CHEOPS mission. YI J.S., CHEN J. and KIPPING D.
2018MNRAS.477..175O 184       D     X         5 42 ~ Constraining planetary migration and tidal dissipation with coeval hot Jupiters. O'CONNOR C.E. and HANSEN B.M.S.
2018MNRAS.478.1763L viz 17       D               3 518 2 The detectability of radio emission from exoplanets. LYNCH C.R., MURPHY T., LENC E., et al.
2019PASP..131c4401D viz 17       D               1 688 ~ Predicted yield of transits of known radial velocity exoplanets from the TESS primary and extended missions. DALBA P.A., KANE S.R., BARCLAY T., et al.
2019MNRAS.489.4311C 17       D               1 43 ~ On the survivability of planets in young massive clusters and its implication of planet orbital architectures in globular clusters. CAI M.X., PORTEGIES ZWART S., KOUWENHOVEN M.B.N., et al.
2020AJ....160..126G 17       D               1 45 ~ TYCHO: realistically simulating exoplanets within stellar clusters. I. Improving the Monte Carlo approach. GLASER J.P., McMILLAN S.L.W., GELLER A.M., et al.
2022ApJ...939...94M 19       D               1 131 ~ New Coronae and Stellar Associations Revealed by a Clustering Analysis of the Solar Neighborhood. MORANTA L., GAGNE J., COUTURE D., et al.

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2023.01.27-19:24:19

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