Showing 1–20 of 44 results
/ Date/ Name
May 8, 2020Unravelling stellar populations in the Andromeda GalaxyJun 15, 2009The evolution of early and late type galaxies in the COSMOS up to z~1.2Dec 14, 2009Do black hole masses scale with classical bulge luminosities only? The case of the two composite pseudobulge galaxies NGC3368 and NGC3489Apr 23, 2012Kinematic Signatures of Bulges Correlate with Bulge Morphologies and Sérsic IndexMay 7, 2014Central rotations of Milky Way Globular ClustersApr 8, 2014Re-growth of stellar disks in mature galaxies: The two component nature of NGC 7217 revisited with VIRUS-WJul 20, 2017Evidence for non-axisymmetry in M31 from wide-field kinematics of stars and gasApr 10, 2018Evidence for the formation of the young counter-rotating stellar disk from gas acquired by IC 719May 27, 2020Following the TraCS of exoplanets with Pan-Planets: Wendelstein-1b and Wendelstein-2bAug 16, 2016K2 Discovers a Busy Bee: An Unusual Transiting Neptune Found in the Beehive ClusterAug 1, 2017The KMOS Cluster Survey (KCS) I: The fundamental plane and the formation ages of cluster galaxies at redshift $1.4<z<1.6$Nov 26, 1998Elliptical Galaxies: Detailed Structure, Scaling Relations and FormationMar 1, 2016Sizes, Colour gradients and Resolved Stellar Mass Distributions for the Massive Cluster Galaxies in XMMUJ2235-2557 at z = 1.39Mar 3, 2016The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3DJun 10, 2020Non-parametric Triaxial Deprojection of Elliptical GalaxiesJun 6, 2019The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^{\rm 3D}$Nov 10, 2014Composite Bulges: The Coexistence of Classical Bulges and Disky Pseudobulges in S0 and Spiral GalaxiesMar 30, 2015First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOSMar 9, 2018Spectroscopic decomposition of NGC 3521: unveiling the properties of the bulge and discMar 22, 2017KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7