open13siWe thank the anonymous referee for useful comments that contributed to improve the presentation of the paper. F.R.F. acknowledges the ESO Visitor Programme for the support and the warm hospitality at the ESO Headquarters in Garching (Germany) during the period when part of this work was performed. A.L.V. acknowledges support from a Marie Sklodowska-Curie Fellowship (MSCA-IF-EFRI 658088).We present the first results of the Multi-Instrument Kinematic Survey of Galactic Globular Clusters (GGCs), a project aimed at exploring the internal kinematics of a representative sample of GGCs from the radial velocity of individual stars, covering the entire radial extension of each system. This is achieved by exploiting the formidable combination...
We present the results from a study of the dynamics of the system of globular clusters around M87. A...
We present wide-field spectroscopy of globular clusters around the Leo I group galaxies NGC 3379 and...
Galactic globular clusters are nearly gas-free, self-gravitating stellar systems characterized by an...
We present the first results of the Multi-Instrument Kinematic Survey of Galactic Globular Clusters ...
As part of the ESO-VLT Multi-Instrument Kinematic Survey of Galactic globular clusters (GCs), we pre...
The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and for...
none27siThe Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin...
We present a spectrophotometric survey of 2522 extragalactic globular clusters (GCs) around 12 early...
In the context of the ESO-VLT Multi-Instrument Kinematic Survey (MIKiS) of Galactic globular cluster...
We present new radial velocity measurements for 82 stars, members of the Galactic globular cluster (...
The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and for...
We present a spectrophotometric survey of 2522 extragalactic globular clusters (GCs) around 12 early...
This is the first of a series of papers presenting the results from our survey of 25 Galactic globul...
Here I present first results from the ESO-VLT Multi-Instrument Kinematic Survey of Galactic Globular...
We derived the three-dimensional velocities of individual stars in a sample of 62 Galactic globular ...
We present the results from a study of the dynamics of the system of globular clusters around M87. A...
We present wide-field spectroscopy of globular clusters around the Leo I group galaxies NGC 3379 and...
Galactic globular clusters are nearly gas-free, self-gravitating stellar systems characterized by an...
We present the first results of the Multi-Instrument Kinematic Survey of Galactic Globular Clusters ...
As part of the ESO-VLT Multi-Instrument Kinematic Survey of Galactic globular clusters (GCs), we pre...
The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and for...
none27siThe Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin...
We present a spectrophotometric survey of 2522 extragalactic globular clusters (GCs) around 12 early...
In the context of the ESO-VLT Multi-Instrument Kinematic Survey (MIKiS) of Galactic globular cluster...
We present new radial velocity measurements for 82 stars, members of the Galactic globular cluster (...
The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and for...
We present a spectrophotometric survey of 2522 extragalactic globular clusters (GCs) around 12 early...
This is the first of a series of papers presenting the results from our survey of 25 Galactic globul...
Here I present first results from the ESO-VLT Multi-Instrument Kinematic Survey of Galactic Globular...
We derived the three-dimensional velocities of individual stars in a sample of 62 Galactic globular ...
We present the results from a study of the dynamics of the system of globular clusters around M87. A...
We present wide-field spectroscopy of globular clusters around the Leo I group galaxies NGC 3379 and...
Galactic globular clusters are nearly gas-free, self-gravitating stellar systems characterized by an...