The role of three-body stability in tidally interacting globular clusters
2014 ◽
Vol 10
(S312)
◽
pp. 231-234
Keyword(s):
AbstractThe role of stability in the general three-body problem is investigated with regard to the tidal radius of a globular cluster (GC) in a galactic potential. This proceedings is a summary of two papers which outline the stability method (Kennedy 2014a) and compare the predicted stability boundary radius to observations of velocity dispersion profiles in Milky Way GCs (Kennedy 2014b).
2018 ◽
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2019 ◽
Vol 14
(S351)
◽
pp. 524-527
2021 ◽
Vol 57
(2)
◽
pp. 311-319
1969 ◽
Vol 33
(1)
◽
pp. 105-110
◽
Keyword(s):
1999 ◽
Vol 172
◽
pp. 291-302
Keyword(s):
Keyword(s):
2014 ◽
Vol 444
(4)
◽
pp. 3328-3339
◽
Keyword(s):
2007 ◽
Vol 135
(1)
◽
pp. 187-195
◽
Keyword(s):