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Titlebook: Measurements of Spin-Orbit Angles for Transiting Systems; Toward an Understand Teruyuki Hirano Book 2014 Springer Japan 2014 Exoplanet.Meas

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發(fā)表于 2025-3-21 17:04:14 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Measurements of Spin-Orbit Angles for Transiting Systems
副標(biāo)題Toward an Understand
編輯Teruyuki Hirano
視頻videohttp://file.papertrans.cn/629/628147/628147.mp4
概述Involves the first detection of the RM effect for a Neptune-sized exoplanet (HAT-P-11b), which showed a significant spin-orbit misalignment..Presents the first discovery of an overlapping event of two
叢書(shū)名稱Springer Theses
圖書(shū)封面Titlebook: Measurements of Spin-Orbit Angles for Transiting Systems; Toward an Understand Teruyuki Hirano Book 2014 Springer Japan 2014 Exoplanet.Meas
描述.This 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 rotation
出版日期Book 2014
關(guān)鍵詞Exoplanet; Measurements of spin-orbit angle; Origin of close-in Planets; Planetary Migration; Planetary
版次1
doihttps://doi.org/10.1007/978-4-431-54586-6
isbn_softcover978-4-431-56189-7
isbn_ebook978-4-431-54586-6Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer Japan 2014
The information of publication is updating

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發(fā)表于 2025-3-21 21:00:05 | 只看該作者
Teruyuki Hirano the value assigned to bankruptcy. Furthermore, the agent’s relative risk aversion in the HARA case inherits the monotonicity behavior from his consumption utility provided his wealth is greater than another boundary level. At smaller wealth levels, however, the relative risk aversion is increasing
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發(fā)表于 2025-3-22 02:55:20 | 只看該作者
Teruyuki Hiranorect for some parameter values and not for others. The problem with Merton‘s solution is that it sometimes violates the constraints against negative wealth and negative consumption stated in Merton (1969) and presumably applicable in Merton (1971 and 1973). This not only affects the solution at the zero-wealt978-1-4613-7871-6978-1-4615-6257-3
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發(fā)表于 2025-3-22 04:54:36 | 只看該作者
Teruyuki Hiranoome parameter values and not for others. The problem with Merton‘s solution is that it sometimes violates the constraints against negative wealth and negative consumption stated in Merton (1969) and presumably applicable in Merton (1971 and 1973). This not only affects the solution at the zero-wealt
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發(fā)表于 2025-3-22 12:25:52 | 只看該作者
Teruyuki Hiranoelative risk aversion is nondecreasing with wealth, while his absolute risk aversion is decreasing with wealth only if he is sufficiently wealthy. At lower wealth levels, however, the agent’s absolute risk aversion may increase with wealth in some cases.
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發(fā)表于 2025-3-22 19:50:10 | 只看該作者
Teruyuki Hiranoome parameter values and not for others. The problem with Merton‘s solution is that it sometimes violates the constraints against negative wealth and negative consumption stated in Merton (1969) and presumably applicable in Merton (1971 and 1973). This not only affects the solution at the zero-wealt
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發(fā)表于 2025-3-22 23:52:30 | 只看該作者
compete in terms of outputs, the free entry equilibrium number of firms exceeds the welfare-maximizing (first-best as well as second-best) number of firms. It follows that the restriction of firm entry so as to prevent the number of firms from exceeding the welfare-maximizing number in accordance wi
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發(fā)表于 2025-3-23 06:02:06 | 只看該作者
New Observations and Improved Analyses of the Rossiter-McLaughlin Effect,g of the anomalous radial velocities during a transit, and hence the systematic errors in . and . reported in the original papers are more or less overlooked. Based on this context, we report the reanalysis of the observed RVs for selected transiting systems for which the RM effect was previously de
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