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All issues Astron. Astrophys. Suppl. Ser., 116 3 (1996) 447-461 Article references

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Cited article:

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A distance of 13 Mpc resolves the claimed anomalies of the galaxy lacking dark matter

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Monthly Notices of the Royal Astronomical Society 486 (1) 1192 (2019)
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The Formation and Evolution of M33 as Revealed by Its Star Clusters

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Springer Theses, The Formation and Evolution of M33 as Revealed by Its Star Clusters 51 (2013)
https://doi.org/10.1007/978-1-4614-7327-5_4

Newly identified star clusters in M33 - III. Structural parameters

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Binaries of massive black holes in rotating clusters: dynamics, gravitational waves, detection and the role of eccentricity

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Hubble Space TelescopeWFPC2 Color-Magnitude Diagrams for Globular Clusters in M31

R. M. Rich, C. E. Corsi, C. Cacciari, et al.
The Astronomical Journal 129 (6) 2670 (2005)
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DYNAMICAL EVOLUTION OF ROTATING SINGLE-MASS STELLAR CLUSTER

ELIANI ARDI, RAINER SPURZEM and SHIN MINESHIGE
Journal of The Korean Astronomical Society 38 (2) 207 (2005)
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The interplay of rotation and relaxation in star clusters and galactic nuclei

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Bright X‐Ray Sources in M31 Globular Clusters

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High Performance Computing in Science and Engineering ’01

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M31 Globular Clusters in the [ITAL]Hubble Space Telescope[/ITAL] Archive. II. Structural Parameters

Pauline Barmby, Stephen Holland and John P. Huchra
The Astronomical Journal 123 (4) 1937 (2002)
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Dynamical evolution of rotating stellar systems -- I. Pre-collapse, equal-mass system

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