The luminosity function of young star clusters: implications for the maximum mass and luminosity of clusters
A&A, 450 1 (2006) 129-145
Published online: 2006-04-03
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https://doi.org/10.1017/S1743921309990809
The Baltimore and Utrecht models for cluster dissolution
Henny J. G. L. M. LamersAstrophysics and Space Science 324 (2-4) 183 (2009)
https://doi.org/10.1007/s10509-009-0125-4
The star cluster population of the spiral galaxy NGC 3370
M. Cantiello, E. Brocato and J. P. BlakesleeAstronomy & Astrophysics 503 (1) 87 (2009)
https://doi.org/10.1051/0004-6361/200912045
What determines the mass of the most massive star cluster in a galaxy: statistics, physics or disruption?
Mark GielesAstrophysics and Space Science 324 (2-4) 299 (2009)
https://doi.org/10.1007/s10509-009-0102-y
Fitting power-law distributions to data with measurement errors
C. Koen and L. KondloMonthly Notices of the Royal Astronomical Society 397 (1) 495 (2009)
https://doi.org/10.1111/j.1365-2966.2009.14956.x