Starspot properties and photometric parameters of transiting planets and their host stars

To begin understanding how the architecture of hot Jupiter planetary systems can be so radically different from that of our own solar system, requires the dynamical evolution of planets to be known. By measuring the sky-projected obliquity � of a system it is possible to determine the dominant proce...

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Bibliographic Details
Main Author: Tregloan-Reed, Jeremy
Published: Keele University 2014
Subjects:
Online Access:http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.676861