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100   $a20140626d2014      u|             0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 10$aMeasurements of Spin-Orbit Angles for Transiting Systems$b[electronic resource] $eToward an Understanding of the Migration History of Exoplanets /$fby Teruyuki Hirano
205   $a1st ed. 2014.
210  1$aTokyo :$cSpringer Japan :$cImprint: Springer,$d2014.
215   $a1 online resource (143 p.)
225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
300   $aDescription based upon print version of record.
311   $a1-322-17347-8 
311   $a4-431-54585-9 
320   $aIncludes bibliographical references at the end of each chapters.
327   $aIntroduction -- Evolution History of Extrasolar Planetary Systems -- Improved Modeling of the Rossiter-McLaughlin Effect -- New Observations and Improved Analyses of the Rossiter-McLaughlin Effect -- Toward the Measurements of Spin-Orbit Relations for Small Planets -- Summary and Future Prospects.
330   $aThis thesis presents accurate analyses of the spin-orbit angle for many remarkable transiting exoplanetary systems, including the first measurement of the Rossiter-McLaughlin effect for a multiple transiting system.   The author presents the observational methods needed to probe the spin-orbit angle, the relation between the stellar spin axis and planetary orbital axis. Measurements of the spin-orbit angle provide us a unique and valuable opportunity to understand the origin of close-in giant exoplanets, called "hot Jupiters".   The first method introduced involves observations of the Rossiter-McLaughlin effect (RM effect). The author points out the issues with the previous theoretical modeling of the RM effect and derives a new and improved theory. Applications of the new theory to observational data are also presented for a number of remarkable systems, and the author shows that the new theory minimizes the systematic errors by applying it to the observational data.   The author also describes another method for constraining the spin-orbit angle: by combining the measurements of stellar flux variations due to dark spots on the stellar surface, with the projected stellar rotational velocity measured via spectroscopy, the spin-orbit angles "along the line-of-sight" are constrained for the transiting exoplanetary systems reported by the Kepler space telescope.
410  0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
606   $aSpace sciences
606   $aPlanetology
606   $aObservations, Astronomical
606   $aAstronomy?Observations
606   $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030
606   $aPlanetology$3https://scigraph.springernature.com/ontologies/product-market-codes/G18010
606   $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014
615  0$aSpace sciences.
615  0$aPlanetology.
615  0$aObservations, Astronomical.
615  0$aAstronomy?Observations.
615 14$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
615 24$aPlanetology.
615 24$aAstronomy, Observations and Techniques.
676   $a521.3
700   $aHirano$b Teruyuki$4aut$4http://id.loc.gov/vocabulary/relators/aut$0792022
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910300371103321
996   $aMeasurements of Spin-Orbit Angles for Transiting Systems$91770902
997   $aUNINA