Titlebook: Characterizing Stellar and Exoplanetary Environments; Helmut Lammer,Maxim Khodachenko Book 2015 The Editor(s) (if applicable) and The Auth

DEVIL

上釉彩

https://doi.org/10.1007/978-3-8348-9468-7tions, discussed in this Chapter, show that the gaseous envelopes around hot Jupiters may be significantly non-spherical and, at the same time, stationary and long-lived. These results are of fundamental importance for the interpretation of observational data.

charisma

,Fertigteile mit Ortbetonergänzung,sphere of a hydrogen-rich exoplanet. Partial deposition rates of the stellar XUV radiation due to the photolytic processes in the . transition region in the upper atmosphere of HD 209458b were calculated. The Monte Carlo model developed by authors was used to calculate the collisional kinetics and t

RALES

摇晃

,Fertigteile mit Ortbetonergänzung,es have claimed that stars with close-in, massive exoplanets are statistically more active, but others conclude that this correlation is just the product of a selection bias. Studies with the Kepler-satellite show that superflares exist, but they do not seem to be caused by the interaction between s

尖牙

梯田

Physikalisch-technisches Grundwissen, limited. For the next decade, the post-HST era, the World Space Observatory UltraViolet (WSO–UV) will be the only large telescope class mission for UV observations, both spectroscopic and imaging. In its potential, the WSO–UV mission is similar to the HST, but all the observing time will be availab

FIS

Helmut Lammer,Maxim KhodachenkoPresents studies of exoplanets under extreme stellar radiation and plasma conditions.Analyzes findings from Hubble Space Telescope observations of transiting exoplanets.Presents applications of advanc

Employee

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