The ACS Virgo Cluster survey. XII. The luminosity function of globular clusters in early-type galaxies

Keyphrases

• Globular Clusters 100%
• Cluster Survey 100%
• Luminosity Function 100%
• Early-type Galaxies 100%
• Virgo Cluster 100%
• Galaxies 47%
• Cluster Mass 23%
• Mass Function 23%
• Galaxy Luminosities 17%
• Low-mass 11%
• Luminosity 11%
• Globular Cluster Systems 11%
• Maximum Likelihood Estimation 5%
• Mass Loss 5%
• Gaussian Representation 5%
• Mass Distribution 5%
• Systematic Variation 5%
• Mass Scale 5%
• Function Model 5%
• Virgo 5%
• Dwarf Galaxies 5%
• Dynamical Evolution 5%
• Hubble Time 5%
• Dynamical Friction 5%
• Starburst 5%
• Massive Galaxies 5%
• Hubble 5%
• Distance Indicators 5%
• Long-term Dynamical Evolution 5%
• Turnover Point 5%
• Two-body 5%
• Evaporation Rate 5%
• Small Variation 5%
• Initial Cluster 5%
• Young Massive Clusters 5%
• Dynamical Mass 5%
• Function Description 5%
• Host Galaxy 5%
• High-mass 5%
• Significant Trends 5%

Physics

• Virgo Cluster 100%
• Luminosity Function 100%
• Early-Type Galaxies 100%
• Globular Cluster 100%
• Galaxy Luminosity 15%
• Gaussian Distribution 10%
• Dynamical Evolution 10%
• Hubble Time 5%
• Dynamical Friction 5%
• Mass Distribution 5%
• Distance Indicators 5%
• Maximum Likelihood Estimate 5%
• Dwarf Galaxy 5%

INIS

• surveys 100%
• luminosity 100%
• galaxies 100%
• variations 21%
• dispersions 15%
• evaporation 10%
• density 5%
• range 5%
• values 5%
• relaxation 5%
• host 5%
• correlations 5%
• friction 5%
• distance 5%
• indicators 5%
• losses 5%
• potentials 5%
• maximum-likelihood fit 5%
• time dependence 5%
• mass loss 5%
• scaling 5%
• probes 5%
• mass distribution 5%
• two-body problem 5%