291 citations · 507 across the 6 of their papers we have counts for
6 papers
Sculpting Andromeda -- made-to-measure models for M31's bar and composite bulge: dynamics, stellar and dark matter mass
Matias Blaña, Ortwin Gerhard, Christopher Wegg +6
The Andromeda galaxy (M31) contains a box/peanut bulge (BPB) entangled with a classical bulge (CB) requiring a triaxial modelling to determine the dynamics, stellar and dark matter…
The stellar populations of the central region of M31
R. P. Saglia, M. Opitsch, M. H. Fabricius +3
We continue the analysis of the dataset of our spectroscopic observation campaign of M31, by deriving simple stellar population properties (age metallicity and alpha-elements overa…
Evidence for non-axisymmetry in M31 from wide-field kinematics of stars and gas
Michael Opitsch, Maximilian H. Fabricius, Roberto P. Saglia +3
As the nearest large spiral galaxy, M31 provides a unique opportunity to learn about the structure and evolutionary history of this galaxy type in great detail. Among the many obse…
Andromeda chained to the Box -- Dynamical Models for M31: Bulge & Bar
Matias Blana, Christopher Wegg, Ortwin Gerhard +5
Andromeda is our nearest neighbouring disk galaxy and a prime target for detailed modelling of the evolutionary processes that shape galaxies. We analyse the nature of M31's triaxi…
The SINFONI Black Hole Survey: The Black Hole Fundamental Plane revisited and the paths of (co-) evolution of supermassive black holes and bulges
R. P. Saglia, M. Opitsch, P. Erwin +7
We investigate the correlations between the black hole mass , the velocity dispersion , the bulge mass , the bulge average spherical density and its spheri…
Central rotations of Milky Way Globular Clusters
Maximilian H. Fabricius, Eva Noyola, Surangkhana Rukdee +6
Most Milky Way globular clusters (GCs) exhibit measurable flattening, even if on a very low level. Both cluster rotation and tidal fields are thought to cause this flattening. Neve…