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NESSY: NEw Science from the phase space of dense stellar SYstems
Heggie, Douglas
(Principal Investigator)
School of Mathematics
Overview
Fingerprint
Research output
(2)
Project Details
Status
Finished
Effective start/end date
1/05/16
→
30/06/19
Funding
UK-based charities:
£177,131.00
View all
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Fingerprint
Explore the research topics touched on by this project. These labels are generated based on the underlying awards/grants. Together they form a unique fingerprint.
rotating spheres
Physics & Astronomy
100%
anisotropy
Earth & Environmental Sciences
85%
star clusters
Physics & Astronomy
77%
kinematics
Earth & Environmental Sciences
65%
stellar systems
Physics & Astronomy
45%
moments
Physics & Astronomy
19%
angular momentum
Earth & Environmental Sciences
13%
globular clusters
Physics & Astronomy
9%
Research output
Research output per year
2017
2017
2019
2019
2
Article
Research output per year
Research output per year
Mapping the stability of stellar rotating spheres via linear response theory
Rozier, S.
,
Fouvry, J-B.
,
Breen, P. G.
,
Varri, A. L.
,
Pichon, C.
&
Heggie, D. C.
,
1 Jul 2019
,
In:
Monthly Notices of the Royal Astronomical Society .
487
,
1
,
p. 711-728
18 p.
Research output
:
Contribution to journal
›
Article
›
peer-review
Open Access
File
rotating spheres
100%
anisotropy
28%
angular momentum
13%
stellar systems
10%
kinematics
9%
The kinematic richness of star clusters - I. Isolated spherical models with primordial anisotropy
Breen, P. G.
,
Varri, A. L.
&
Heggie, D. C.
,
1 Nov 2017
,
In:
Monthly Notices of the Royal Astronomical Society .
471
,
3
,
p. 2778-2789
Research output
:
Contribution to journal
›
Article
›
peer-review
Open Access
star clusters
100%
anisotropy
73%
kinematics
73%
stellar systems
44%
moments
24%