Showing 1–20 of 98 results
/ Date/ Name
Feb 25, 1997The shape of galaxy disks: how the scale height increases with galactocentric distanceJul 7, 1997The z-structure of disk galaxies towards the galaxy planesAug 31, 2018Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV dataSep 10, 2010Near-infrared and optical observations of galactic warps: A common, unexplained feature of most discsSep 4, 2003Young star clusters: Clues to galaxy formation and evolutionFeb 29, 2016The VMC Survey. XIX. Classical Cepheids in the Small Magellanic CloudMar 23, 2015The VMC survey - XV. The Small Magellanic Cloud--Bridge connection history as traced by their star cluster populationsJun 10, 2014Eclipsing binary stars in the Large Magellanic Cloud. Results from the EROS-2, OGLE and VMC surveysOct 25, 2013The VMC Survey - X. Cepheids, RR Lyrae stars and binaries as probes of the Magellanic System's structureSep 23, 2005The initial mass distribution of the M82 star cluster systemFeb 15, 2005Systematic uncertainties in the analysis of star cluster parameters based on broad-band imaging observationsApr 22, 2005From young massive star cluster to old globular: the L_V-sigma_0 relationship as a diagnostic toolMay 3, 2006HST/STIS Spectroscopy of Five Super Star Clusters in the Starburst Galaxy M82Dec 11, 2007The effect of binaries on the dynamical mass determination of star clustersOct 5, 2007Binaries and the dynamical mass of star clustersJun 27, 2014The VMC ESO Public SurveySep 9, 2014How does a low-mass cut-off in the stellar IMF affect the evolution of young star clusters?Aug 7, 2002Mass segregation in rich clusters in the Large Magellanic Cloud - III. Implications for the initial mass functionJul 8, 2002On the nature of a secondary main sequence turn-off in the rich LMC cluster NGC 1868Feb 14, 2003Star Cluster Formation and Evolution in Nearby Starburst Galaxies: I. Systematic Uncertainties