Accurate Stellar Parameters for Radial Velocity Surveys

Living reference work entry

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.

Notes

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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Copyright information

© Springer International Publishing AG, part of Springer Nature 2018

Authors and Affiliations

  1. 1.Instituto de Astrofísica e Ciências do EspaçoUniversidade do Porto, CAUPPortoPortugal
  2. 2.Departamento de Física e AstronomiaFaculdade de Ciências, Universidade do PortoPortoPortugal
  3. 3.Centre for Star and Planet Formation, Natural History Museum of Denmark & Niels Bohr InstituteUniversity of CopenhagenCopenhagen KDenmark

Section editors and affiliations

  • Hans Kjeldsen
    • 1
  1. 1.Stellar Astrophysics CentreAarhus UniversityAarhusDenmark

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