tests:collision:new_challenges
Differences
This shows you the differences between two versions of the page.
Both sides previous revisionPrevious revisionNext revision | Previous revision | ||
tests:collision:new_challenges [2014/11/13 14:56] – v.henault-brunet | tests:collision:new_challenges [2022/10/24 12:27] (current) – external edit 127.0.0.1 | ||
---|---|---|---|
Line 1: | Line 1: | ||
====== Ideas for additional challenges ====== | ====== Ideas for additional challenges ====== | ||
+ | |||
+ | ===== Weighing dark remnants using luminous stars ===== | ||
+ | Explore how/if the mass function of dark remnants can be constrained from a limited set of observables, | ||
+ | |||
+ | |||
+ | ===== Dark remnants & IMBH ===== | ||
+ | Laura is applying her discrete Jeans modelling method to snapshots of N-body models that contain stellar-mass black holes. The idea is check if a concentration of dark remnants near the centre can be mistaken for an intermediate-mass black hole. | ||
+ | |||
===== Pal 5 model from Andreas Kuepper in streams section ===== | ===== Pal 5 model from Andreas Kuepper in streams section ===== |
tests/collision/new_challenges.1415890571.txt.gz · Last modified: 2022/10/24 12:26 (external edit)