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The dynamics of these objects, if they do exist, must be quite different from that of standard star clusters. With a very narrow mass range (all brown dwarfs or white dwarfs), the evaporation rate of these RAMBOs should be very slow as predicted by the evolution of simulated mono-component cluster
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models. Theoretically, these very long-lived objects could exist in large numbers. The presence of a clustered thick disk-like component of
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has been suggested by
Sanchez-Salcedo (1997, 1999) and Kerins (1997).
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in 1995. They may have an effective radius between 1 and 15
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241:Monthly Notices of the Royal Astronomical Society
18:Robust association of massive baryonic objects
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69:, with masses in the range 10–100,000
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7:
155:Weakly interacting massive particles
61:RAMBOs were proposed by Moore and
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174:Moore, B., & Silk, J. 1995,
190:de la Fuente Marcos, R. 1995,
40:robust association of massive
1:
238:Sánchez-Salcedo, F. J. 1999,
222:Sánchez-Salcedo, F. J. 1997,
27:Proposed type of star cluster
226:, 487, L61-L64 (ADS entry
149:Massive compact halo object
144:Hypercompact stellar system
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244:, 303, 755-772 (ADS entry
210:, 322, 709-718 (ADS entry
208:Astronomy and Astrophysics
194:, 301, 407-418 (ADS entry
192:Astronomy and Astrophysics
85:referencing the character
178:, 442, L5-L8 (ADS entry
224:Astrophysical Journal
176:Astrophysical Journal
206:Kerins, E. J. 1997,
83:contrived acronym
16:(Redirected from
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81:The name is a
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269:Open clusters
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139:Microlensing
134:White dwarfs
129:Brown dwarfs
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56:white dwarfs
52:brown dwarfs
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124:Dark matter
108:dark matter
258:Categories
162:References
87:John Rambo
46:is a dark
32:astronomy
151:(MACHOs)
118:See also
101:Dynamics
75:☉
50:made of
42:baryonic
157:(WIMPs)
110:in the
93:" and "
67:parsecs
48:cluster
44:objects
112:Galaxy
91:MACHO
36:RAMBO
95:WIMP
63:Silk
34:, a
97:".
54:or
38:or
30:In
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72:M
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