tests:collision:new_challenges
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tests:collision:new_challenges [2014/10/22 15:14] – v.henault-brunet | tests:collision:new_challenges [2022/10/24 12:27] (current) – external edit 127.0.0.1 | ||
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====== Ideas for additional challenges ====== | ====== Ideas for additional challenges ====== | ||
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+ | ===== Weighing dark remnants using luminous stars ===== | ||
+ | Explore how/if the mass function of dark remnants can be constrained from a limited set of observables, | ||
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+ | |||
+ | ===== 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. | ||
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===== Pal 5 model from Andreas Kuepper in streams section ===== | ===== Pal 5 model from Andreas Kuepper in streams section ===== | ||
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- | ===== Snapshots of an N-body model of M4 ===== | + | ===== Mass modelling multiple-population GC with non-parametric method===== |
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+ | Apply Pascal Steger' | ||
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+ | The data has the following format. | ||
+ | ^ $m$ ^ $x$ ^ $y$ ^ $z$ ^ $v_x$ ^ $v_y$ ^ $v_z$ ^ population ^ | ||
+ | | [Msun] | [pc] |[pc]|[pc]| [km/s] | [km/ | ||
- | As another source of mock data, snapshots from a large N-body simulation of the globular cluster M4 are [[http:// | + | |
tests/collision/new_challenges.1413990881.txt.gz · Last modified: 2022/10/24 12:26 (external edit)