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Cited article:

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Monthly Notices of the Royal Astronomical Society: Letters 476 (1) L29 (2018)
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Gas Expulsion in MOND: The Possible Origin of Diffuse Globular Clusters and Ultra-faint Dwarf Galaxies

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A Universal Velocity Dispersion Profile for Pressure Supported Systems: Evidence for MONDian Gravity across Seven Orders of Magnitude in Mass

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Application of three-body stability to globular clusters – II. Observed velocity dispersions

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Monthly Notices of the Royal Astronomical Society 445 (4) 4443 (2014)
https://doi.org/10.1093/mnras/stu2038

Mass segregation in the outer halo globular cluster Palomar 14

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THE MOND EXTERNAL FIELD EFFECT ON THE DYNAMICS OF THE GLOBULAR CLUSTERS: GENERAL CONSIDERATIONS AND APPLICATION TO NGC 2419

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The Astrophysical Journal 783 (1) 48 (2014)
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The dynamical phase transitions of stellar systems and the corresponding kinematics

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A MONTE CARLO ANALYSIS OF THE VELOCITY DISPERSION OF THE GLOBULAR CLUSTER PALOMAR 14

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Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions

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Living Reviews in Relativity 15 (1) (2012)
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The velocity dispersion and mass function of the outer halo globular cluster Palomar 4

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Modifying gravity: you cannot always get what you want

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Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 369 (1957) 5018 (2011)
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POLYTROPIC MODEL FITS TO THE GLOBULAR CLUSTER NGC 2419 IN MODIFIED NEWTONIAN DYNAMICS

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The Astrophysical Journal 743 (1) 43 (2011)
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Testing Newtonian gravity with distant globular clusters: NGC 1851 and NGC 1904 

R. Scarpa, G. Marconi, G. Carraro, R. Falomo and S. Villanova
Astronomy & Astrophysics 525 A148 (2011)
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Direct N-body simulations of globular clusters - I. Palomar 14

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