Add to ORKGWe report on ongoing photometric and spectroscopic work on a sample of isolated elliptical galaxies. We investigate their globular cluster systems, and use the kinematics of globular clusters and the integrated galaxy light to constrain their dark halos, which are not found in the cases of NGC 5812 and NGC 7507.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plat
The dark matter (DM) halos of field elliptical galaxies have not been well-studied and their propert...
Ellipticals in very low density environments are extremely rare but hold important clues about galax...
In this paper we consider three-integral axisymmetric models for NGC 4649 and NGC 7097, addressing t...
Context. Rich globular cluster systems, particularly the metal-poor part of them, are thought to be ...
Context. Rich globular cluster systems, particularly the metal-poor part of them, are thought to be ...
Context. There is strong evidence that globular cluster systems (GCSs) of massive galaxies are large...
The dark matter (DM) halos of field elliptical galaxies have not been well-studied and their propert...
The globular cluster (GC) systems of isolated elliptical galaxies have only recently begun to be stu...
We investigate the distribution of the luminous and the dark matter components in the isolated ellip...
I present various projects to study the halo dynamics of elliptical galaxies. This allows one to stu...
As tracers of star formation, galaxy assembly, and mass distribution, globular clusters have provide...
Context. Previous studies have shown that the kinematics of the field elliptical galaxy NGC 7507 do ...
The kinematics of the outer parts of three intermediate-luminosity elliptical galaxies were studied ...
The dark matter (DM) halos of field elliptical galaxies have not been well-studied and their propert...
Context. There is strong evidence that globular cluster systems (GCSs) of massive galaxies are large...
The dark matter (DM) halos of field elliptical galaxies have not been well-studied and their propert...
Ellipticals in very low density environments are extremely rare but hold important clues about galax...
In this paper we consider three-integral axisymmetric models for NGC 4649 and NGC 7097, addressing t...
Context. Rich globular cluster systems, particularly the metal-poor part of them, are thought to be ...
Context. Rich globular cluster systems, particularly the metal-poor part of them, are thought to be ...
Context. There is strong evidence that globular cluster systems (GCSs) of massive galaxies are large...
The dark matter (DM) halos of field elliptical galaxies have not been well-studied and their propert...
The globular cluster (GC) systems of isolated elliptical galaxies have only recently begun to be stu...
We investigate the distribution of the luminous and the dark matter components in the isolated ellip...
I present various projects to study the halo dynamics of elliptical galaxies. This allows one to stu...
As tracers of star formation, galaxy assembly, and mass distribution, globular clusters have provide...
Context. Previous studies have shown that the kinematics of the field elliptical galaxy NGC 7507 do ...
The kinematics of the outer parts of three intermediate-luminosity elliptical galaxies were studied ...
The dark matter (DM) halos of field elliptical galaxies have not been well-studied and their propert...
Context. There is strong evidence that globular cluster systems (GCSs) of massive galaxies are large...
The dark matter (DM) halos of field elliptical galaxies have not been well-studied and their propert...
Ellipticals in very low density environments are extremely rare but hold important clues about galax...
In this paper we consider three-integral axisymmetric models for NGC 4649 and NGC 7097, addressing t...