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RT @NatureAstronomy: No need for binary black holes to explain the puffed-up sizes of old star clusters in the LMC. The right initial condi…
RT @NatureAstronomy: No need for binary black holes to explain the puffed-up sizes of old star clusters in the LMC. The right initial condi…
Size diversity of old Large Magellanic Cloud clusters as determined by internal dynamical evolution https://t.co/avcpSYkGgp via @NatureAstronomy https://t.co/aKIS8VJcyW
No need for binary black holes to explain the puffed-up sizes of old star clusters in the LMC. The right initial conditions and an energetic dynamical evolution can produce the observed size diversity. Ferraro et al.: https://t.co/6m3OW5bXF3 https://t.co/Z