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标题：Sectoral r modes and periodic radial velocity variations of Sun-like stars
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作者：A. F. Lanza ; L. Gizon ; T. V. Zaqarashvili 等
期刊名称：Astronomy & Astrophysics
印刷版ISSN：0004-6361
电子版ISSN：1432-0746
出版年度：2019
卷号：623
DOI：10.1051/0004-6361/201834712
语种：English
出版社：EDP Sciences
摘要：Context.Radial velocity (RV) measurements are used to search for planets orbiting late-type main-sequence stars and to confirm the transiting planets.Aims.The most advanced spectrometers are now approaching a precision of ~10 cm s−1, which implies the need to identify and correct for all possible sources of RV oscillations intrinsic to the star down to this level and possibly beyond. The recent discovery of global-scale equatorial Rossby waves in the Sun, also calledrmodes, prompted us to investigate their possible signature in stellar RV measurements. Thesermodes are toroidal modes of oscillation whose restoring force is the Coriolis force; they propagate in the retrograde direction in a frame that co-rotates with the star. The solarrmodes with azimuthal orders 3 ≤m≲ 15 were identified unambiguously because of their dispersion relation and their long e-folding lifetimes of hundreds of days.Methods.In this paper, we simulate the RV oscillations produced by sectoralrmodes with 2 ≤m≤ 5 by assuming a stellar rotation period of 25.54 days and a maximum amplitude of the surface velocity of each mode of 2 m s−1. This amplitude is representative of the solar measurements except for them= 2 mode, which has not yet been observed on the Sun.Results.Sectoralrmodes with azimuthal ordersm= 2 and 3 would produce RV oscillations with amplitudes of 76.4 and 19.6 cm s−1and periods of 19.16 and 10.22 days, respectively, for a star with an inclination of the rotation axis to the line of sighti= 60°. Therefore, they may produce rather sharp peaks in the Fourier spectrum of the radial velocity time series that could lead to spurious planetary detections.Conclusions.Sectoralrmodes may represent a source of confusion in the case of slowly rotating inactive stars that are preferential targets for RV planet search. The main limitation of the present investigation is the lack of observational constraints on the amplitude of them= 2 mode on the Sun.
关键词：Key wordsentechniques: radial velocitiesSun: oscillationsstars: oscillationsstars: late-typeplanets and satellites: detectionplanets and satellites: terrestrial planets