Showing 21–40 of 44 results
/ Date/ Name
May 6, 2014Redshift evolution of the dynamical properties of massive galaxies from SDSS-III/BOSSMar 2, 2026Triaxial Schwarzschild Models of Brightest Cluster Galaxies with Long-Slit LBT DataFeb 24, 2009Frequency and properties of bars in cluster and field galaxies at intermediate redshiftsOct 8, 2009Evolution of the Early-Type Galaxy Fraction in Clusters since z = 0.8May 31, 2022Intrinsic shapes of Brightest Cluster GalaxiesOct 7, 2013Searching for transits in the WTS with difference imaging light curvesMay 26, 2014A Consistent Study of Metallicity Evolution at 0.8 < z < 2.6Sep 26, 2017NGC 307 and the Effects of Dark-Matter Haloes on Measuring Supermassive Black Holes in Disc GalaxiesSep 30, 1997Spectroscopic Gradients in Early -- Type Galaxies and Implications on Galaxy FormationMay 20, 2005VLT Spectroscopy of Globular Cluster Systems, II. Spectroscopic Ages, Metallicities, and [alpha/Fe] Ratios of Globular Clusters in Early-Type GalaxiesMar 18, 2024Triaxial Schwarzschild Models of NGC 708: a 10-billion solar mass black hole in a low dispersion galaxy with a Kroupa IMFJul 28, 2015The properties and the formation mechanism of the stellar counter-rotating components in NGC 4191Dec 3, 2025Eight New Ultramassive Black Hole Masses confirm Best Correlation with Galaxy Core SizesOct 4, 2022Accuracy and precision of triaxial orbit models II: Viewing angles, shape and orbital structureSep 2, 2010The central black hole mass of the high-sigma but low-bulge-luminosity lenticular galaxy NGC 1332Sep 12, 2002Integrated Spectroscopy of Bulge Globular Clusters and Fields I. The Data Base and Comparison of Individual Lick Indices in Clusters and BulgeOct 12, 2006The build-up of the colour-magnitude relation in galaxy clusters since z~0.8Feb 12, 2008Dark matter content and internal dynamics of NGC 4697: NMAGIC particle models from slit data and planetary nebulae velocitiesFeb 1, 2008Spectroscopy of clusters in the ESO distant cluster survey (EDisCS).II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fieldsDec 15, 1997The kinematically peculiar cores of the Coma cluster early -- type galaxies NGC 4816 and IC 4051