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Galactic Globular Clusters: A new catalog of masses, structural parameters, velocity dispersion profiles, proper motions and space orbits

Published online by Cambridge University Press:  11 March 2020

Michael Hilker
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748Garching, Germany email: [email protected]
Holger Baumgardt
Affiliation:
School of Mathematics and Physics, The University of Queensland, St. Lucia, QLD 4072, Australia email: [email protected]
Antonio Sollima
Affiliation:
INAF Osservatorio Astronomico di Bologna, via Gobetti 93/3, I-Bologna 40129, Italy email: [email protected]
Andrea Bellini
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: [email protected]
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Abstract

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We collected radial velocities of more than 50.000 individual stars in 156 Galactic globular clusters (GGC) and matched them with HST photometry and Gaia DR2 proper motions. This allowed us to derive the GGC’s mean proper motions and space velocities. By fitting a large set of N-body simulations to their velocity dispersion and surface density profiles, combined with new measurements of their internal radially dependent mass functions, we have determined their present-day masses and structural parameters, and for 144 GGCs their internal kinematics. We also derive the initial cluster masses by calculating the cluster orbits backwards in time applying suitable recipes to account for mass-loss and dynamical friction. The new fundamental parameters of GGCs are publicly available via an online database, which will regularly be updated.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

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