THE OBSERVATIONAL AND THEORETICAL TIDAL RADII OF GLOBULAR CLUSTERS IN M87
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/746/i=1/a=93/pdf
Reference46 articles.
1. Structural Parameters for Globular Clusters in M31 and Generalizations for the Fundamental Plane
2. Evidence for two populations of Galactic globular clusters from the ratio of their half-mass to Jacobi radii
3. The Construction of Nonspherical Models of Quasi‐Relaxed Stellar Systems
4. The inner halo of M 87: a first direct view of the red-giant population
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1. Globular cluster scale sizes in giant galaxies: orbital anisotropy and tidally underfilling clusters in M87, NGC 1399 and NGC 5128;Monthly Notices of the Royal Astronomical Society;2016-05-12
2. The effects of orbital inclination on the scale size and evolution of tidally filling star clusters;Monthly Notices of the Royal Astronomical Society;2014-10-08
3. WIDE-FIELDHUBBLE SPACE TELESCOPEOBSERVATIONS OF THE GLOBULAR CLUSTER SYSTEM IN NGC 1399;The Astrophysical Journal;2014-04-17
4. GLOBULAR CLUSTER SCALE SIZES IN GIANT GALAXIES: THE CASE OF M87 AND THE ROLE OF ORBITAL ANISOTROPY AND TIDAL FILLING;The Astrophysical Journal;2013-11-27
5. The state of globular clusters at birth: emergence from the gas-embedded phase;Monthly Notices of the Royal Astronomical Society;2013-10-26
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