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- W2794266745 abstract "As mentioned in Chap. 1, stars hosting hot Jupiters exhibit a wide range of obliquities. The knowledge comes from the spectroscopic technique, that is, 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 provide complimentary information on those planets. In this chapter, we review the methods to measure stellar obliquities and summarize our current knowledge from observations. The implications for the formation scenario of hot Jupiters will be discussed in the next chapter." @default.
- W2794266745 created "2018-03-29" @default.
- W2794266745 creator A5016518617 @default.
- W2794266745 date "2018-01-01" @default.
- W2794266745 modified "2023-09-27" @default.
- W2794266745 title "Measurements of Stellar Obliquities" @default.
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- W2794266745 doi "https://doi.org/10.1007/978-981-10-8453-9_2" @default.
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