HD 41004Bb , the SIMBAD biblio

HD 41004Bb , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.08.10CEST02:17:55


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Title First 3 Authors
2020MNRAS.492.5141Z 50           X         1 19 ~ Activity and differential rotation of the early M dwarf Kepler-45 from transit mapping. ZALESKI S.M., VALIO A., CARTER B.D., et al.
2019MNRAS.487.3356S 47           X         1 9 ~ Study of the mass-ratio distribution of spectroscopic binaries - II. The boundaries of the brown-dwarf desert as seen with the APOGEE spectroscopic binaries. SHAHAF S. and MAZEH T.
2017AJ....153..148A 62       D     X         2 3 4 Secular orbit evolution in systems with a strong external perturber - A simple and accurate model. ANDRADE-INES E. and EGGL S.
2016MNRAS.462..429G 43           X         1 5 1 On stability of planetary motion during stellar approaches. GASANOV S.A. and MAMMADLI A.H.
2015ApJ...799..147J 126           X         3 13 14 On the likelihood of planet formation in close binaries. JANG-CONDELL H.
2015MNRAS.446.2560M 17       D               1 51 24 Limits on low-frequency radio emission from southern exoplanets with the Murchison Widefield Array. MURPHY T., BELL M.E., KAPLAN D.L., et al.
2015MNRAS.448.3797F 167     A D     X         5 13 2 Can there be additional rocky planets in the Habitable Zone of tight binary stars with a known gas giant? FUNK B., PILAT-LOHINGER E. and EGGL S.
2013A&A...552A.119S viz 16       D               1 1488 42 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2012ApJ...754..137M 42           X         1 14 29 On the detectability of star-planet interaction. MILLER B.P., GALLO E., WRIGHT J.T., et al.
2012ApJ...757....6H 16       D               1 76 32 Calibration of equilibrium tide theory for extrasolar planet systems. II. HANSEN B.M.S.
2012MNRAS.427..397S 16       D               1 36 10 Stability of the Lagrangian point L4 in the spatial restricted three-body problem - application to exoplanetary systems. SCHWARZ R., BAZSO A., ERDI B., et al.
2011A&A...533A..83B 40           X         1 36 60 SOPHIE velocimetry of Kepler transit candidates. III. KOI-423b: an 18 MJup transiting companion around an F7IV star. BOUCHY F., BONOMO A.S., SANTERNE A., et al.
2011ApJ...733...68B viz 16       D               1 308 7 Density estimation for projected exoplanet quantities. BROWN R.A.
2010A&A...509A.103S 39         O X         1 63 14 Hipparcos preliminary astrometric masses for the two close-in companions to HD 131664 and HD 43848. A brown dwarf and a low-mass star. SOZZETTI A. and DESIDERA S.
2010ApJ...709..168A viz 16       D               1 421 68 How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits. ANGLADA-ESCUDE G., LOPEZ-MORALES M. and CHAMBERS J.E.
2010ApJ...722.1547S 94       D       C       3 36 36 Possible constraints on exoplanet magnetic field strengths from planet-star interaction. SCHARF C.A.
2010ApJS..186...48J 16       D               1 175 7 On the fundamental mass-period functions of extrasolar planets. JIANG I.-G., YEH L.-C., CHANG Y.-C., et al.
2010MNRAS.406.1918D 16       D               1 404 29 The Hill stability of the possible moons of extrasolar planets. DONNISON J.R.
2009MNRAS.394L..93M 39           X         1 12 7 On the various origins of close-in extrasolar planets. MARCHI S., ORTOLANI S., NAGASAWA M., et al.
2007A&A...462..345D         O           96 133 Properties of planets in binary systems. The role of binary separation. DESIDERA S. and BARBIERI M.
2007A&A...475..359G viz 15       D               193 59 Predicting low-frequency radio fluxes of known extrasolar planets. GRIESSMEIER J.-M., ZARKA P. and SPREEUW H.
2007ApJ...661.1180O 8 7 119 Tidal dissipation in rotating solar-type stars. OGILVIE G.I. and LIN D.N.C.
2007ApJ...666..475M viz 15       D               185 19 Extrasolar planet taxonomy: a new statistical approach. MARCHI S.
2006ApJ...646..505B viz 16       D               325 672 Catalog of nearby exoplanets. BUTLER R.P., WRIGHT J.T., MARCY G.W., et al.

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2020.08.10-02:17:55

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