The Low Mass X Ray Binary and Globular Cluster Connection in Virgo Cluster Early Type Galaxies: Optical Properties

but no common halo able to reproduce simultaneously the properties of red and blue GCs velocities of some blue GCs require very large apogalactic distances – recent

Globular clusters : deficit of low-mass stars increases with decreasing concentration disagrees with dynamical evolution (Marks et al.. Kroupa: University of Bonn /

The circularized stellar mass density profiles for the galaxies in our sample, comparing them with similar mass SDSS ETGs and the massive compact galaxies in Szomoru et al..

For a given metallicity, the changes in the emission-line spectrum and in the ionization parameter are due to the changes in the cluster mass, which determines the number of

Many of the cluster members are detected, including some embedded, very low-mass objects, several protostars (some of them extended), and substantial emission from the

In this work we use optical imaging and integral field spec- troscopy (IFS) to study the impact of the minor merger on the star formation properties of the individual galaxies of

Relationship between the total cluster stellar mass and the photometric blue fraction for the ALHAMBRA cluster and group sample stacked into different redshift bins. The galaxy

We introduce a toy model that describes (in a single equation) how much baryonic mass is accreted and retained into galaxies as a function of halo mass and redshift. In our model,