Sushan Konar, Mihir Arjunwadkar
Published 2014-02-07, updated 2014-11-26Version 2
There appears to be more than one statistically different populations in the energy distribution of glitches, strongly indicative of different mechanisms accessing different energy ranges responsible for them.
Comments: 2 pages, 1 figure, uses basi.cls, ASI Conference Series on "The Metrewavelength Sky", final version
On the maximum helium content of multiple populations in the globular cluster NGC6752
The role of cluster age on the onset of multiple populations in stellar clusters
The internal kinematics of NGC 2808 and its multiple populations
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