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THE ACS FORNAX CLUSTER SURVEY. IX. THE COLOR-MAGNITUDE RELATION OF GLOBULAR CLUSTER SYSTEMSBased on observations with the NASA/ESA Hubble Space Telescope obtained at the Space Telescope Science Institute, which is operated by the association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.
Online Contents | 2010| -
An extreme IMF as an explanation for high M/L ratios in UCDs? The CO index as a tracer of bottom heavy IMFs
Free accessArXiv | 2007| -
How tidal erosion has shaped the relation between globular cluster specific frequency and galaxy luminosity
Free accessArXiv | 2014| -
THE ACS VIRGO CLUSTER SURVEY. XIV. ANALYSIS OF COLOR-MAGNITUDE RELATIONS IN GLOBULAR CLUSTER SYSTEMS
Online Contents | 2006| -
Dissolution is the solution: on the reduced mass-to-light ratios of Galactic globular clusters
Free accessArXiv | 2009| -
Dynamical versus Stellar Masses of Ultracompact Dwarf Galaxies in the Fornax Cluster
Free accessArXiv | 2010| -
Ultra Compact Objects in the Fornax Cluster of Galaxies: Globular clusters or dwarf galaxies?
Free accessArXiv | 2002| -
Faint dwarf spheroidals in the Fornax Cluster: A flat luminosity function
Free accessArXiv | 2002| -
Dozens of compact and high velocity-dispersion early-type galaxies in Sloan Digital Sky Survey
Free accessArXiv | 2015|
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