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Sensitivity of the orbital content of a model stellar system to the potential approximation used to describe it
(Springer, 2006-10)
We have classified orbits in a stationary triaxial stellar system created from a cold dissipationless collapse of 100,000 particles. In order to integrate the orbits, two potential approximations with different fitting ...
Supernovae: Where and why do they break off?
(SABER ULA, 2005)
Unresolved versus resolved: testing the validity of young simple stellar population models with VLT/MUSE observations of NGC 3603
(EDP Sciences, 2016)
Context. Stellar populations are the building blocks of galaxies, including the Milky Way. The majority, if not all, extragalactic studies are entangled with the use of stellar population models given the unresolved nature ...
Modest 15 - Modelling And Observing Dense Stellar Systems - International Conference
(2017)
he Theory Group at the Departamento de Astronom ıa at the Universidad de Concepci on will organise the MODEST 15 conference, which will be held in Concepci on, Chile at the 2nd - 6th of March 2015.
This will be the 15th ...
Regular and chaotic orbits in a self-consistent triaxial stellar system with slow figure rotation
(Springer, 2006-10)
We created a self-consistent triaxial stellar system through the cold disipationless collapse of 100,000 particles whose evolution was followed with a multipolar code. The resulting system rotates slowly even though its ...
The AIMSS Project, III : the stellar populations of compact stellar systems
(Wiley Blackwell Publishing, Inc, 2016-02)
In recent years, a growing zoo of compact stellar systems (CSSs) have been found whose physical properties (mass, size, velocity dispersion) place them between classical globular clusters (GCs) and true galaxies, leading ...