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...
Main Author: | Tregloan-Reed, Jeremy |
---|---|
Published: |
Keele University
2014
|
Subjects: | |
Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.676861 |
Similar Items
-
Laboratory measurements of ammonia ice and ammonium hydrosulphide ice for use in Jovian radiative transfer models
by: Howett, Carly Jacqueline Amy
Published: (2005) -
Magnetosphere-ionosphere coupling currents in Jupiter's middle magnetosphere
by: Nichols, Jonathan D.
Published: (2004) -
Large-scale current systems in the Jovian magnetosphere
by: Bunce, Emma J.
Published: (2001) -
Fundamental properties of solar-type eclipsing binary stars, and kinematic biases of exoplanet host stars
by: Hutcheon, Richard J.
Published: (2015) -
The influence of environment on the star formation properties of galaxies
by: Rodríguez Del Pino, Bruno
Published: (2015)