A full-lifetime planetary simulation: from stellar birth cluster evolution to planetary destruction around white dwarfs

As such, when stellar encounters inject AMD into the outskirts of planetary systems, outer planetary sys- tems in Model J need to share their AMD with inner plan- ets, whereas in

Vertical profile of radiation dose (Gy), caused by proton spectrum imitating GLE 43 (a)(b) and Carrington Flare (c)(d) penetrating CO 2 rich (terrestrial type) atmosphere on

Specifically, Section 6.1 reflects on the find- ings from Section 2 of this thesis on whether White Dwarfs could have Earth-like planets on which life could form; Sec- tion

License: Licence agreement concerning inclusion of doctoral thesis in the Institutional Repository of the University of Leiden Downloaded from: https://hdl.handle.net/1887/3740..

Although much has been learned about the dynamical structure of stellar systems by modeling their observed surface brightness and kinematics with solutions of the con- tinuity

The black curves are contours of constant mass density in steps of one magnitude, for the input Abel model (solid) and for the fitted Schwarzschild model (dashed). C HAPTER 4: F

Als slachtoffers dezelfde bescherming zouden hebben gekregen als daders, zouden zij nooit slachtoffers zijn

The solutions for the mean streaming motions, i.e., the first velocity moments of the distribution function, are quite helpful in understanding the variety of observed velocity