Abstract
The radial velocity (RV) method has provided a large and increasing number of planets orbiting other suns. Together with the successes of ground- and space-based photometry, RVs allow us to routinely characterize in unique detail thousands of exoplanets. In this chapter, we address some of the main challenges and limitations of the RV method, specially those connected with the properties of the planet host stars. However, we also show that the study of stars with planets, specially those detected or characterized through RVs, is providing unique information about the processes of planet formation, evolution, and composition. Finally, the bright future of this method is highlighted.
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Acknowledgements
This work was supported by Fundação para a Ciência e a Tecnologia (FCT, Portugal) through the research grant through national funds and by FEDER through COMPETE2020 by grants UID/FIS/04434/2013 & POCI-01-0145-FEDER-007672 and PTDC/FIS-AST/1526/2014 & POCI-01-0145-FEDER-016886. N.C.S. acknowledge support from FCT through Investigador FCT contract nr. IF/00169/2012/CP0150/CT0002.
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Santos, N.C., Buchhave, L.A. (2018). Accurate Stellar Parameters for Radial Velocity Surveys. In: Deeg, H., Belmonte, J. (eds) Handbook of Exoplanets . Springer, Cham. https://doi.org/10.1007/978-3-319-30648-3_181-1
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