palpitate 发表于 2025-3-23 12:15:23
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Waqar Zia,Michel Sarkis,Klaus Diepold, modeling of the Rossiter-McLaughlin (RM) effect in the radial velocity (RV) times series. While the RM effect is difficult to observe for planets with smaller radii or on wider orbits than hot Jupiters, new methods based on the high-precision photometric data have recently been developed to providGraphite 发表于 2025-3-24 00:44:43
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Face Localization and Enhancementerence between orbital inclination (almost .) and stellar inclination ., is used to infer the degree of the spin–orbit misalignment. In this chapter, we develop a methodology for determining true stellar obliquity ., combining the analyses of asteroseismology, transit light curves, and the Rossiter–Blanch 发表于 2025-3-24 07:32:09
Jacques Berleur,Tanguy Ewbank de Wespinle by applying the gravity-darkening method (Sect. .) to existing data of transiting systems obtained by the . space telescope. The methodology, however, is not fully established, given the discrepancy between this method and the spectroscopic one recently reported for the hot Jupiter system Kepler-连累 发表于 2025-3-24 11:43:48
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Springer Series in Vision Researchissues that are important to clarify the role of orbital evolution due to dynamical processes: (i) obliquities of stars hosting long-period transiting planets, (ii) origin of intermediate-period giant planets (warm Jupiters) on eccentric orbits, and (iii) possible difference between single- and multNeonatal 发表于 2025-3-24 19:29:38
Springer Series in Vision Researchissues that are important to clarify the role of orbital evolution due to dynamical processes: (i) obliquities of stars hosting long-period transiting planets, (ii) origin of intermediate-period giant planets (warm Jupiters) on eccentric orbits, and (iii) possible difference between single- and multi-transiting systems.Chauvinistic 发表于 2025-3-24 23:41:54
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