Context. Aims. We derive rotation curves from optical emission lines of 182 disc galaxies (96 in the cluster and 86 in the field) in the region of Abell 901/902 located at z ~ 0.165. We continue the kinematic analysis presented in a previous paper. Here
The research presented in this Ph.D thesis is mainly focused on the Tully– Fisher relation as a tool...
In this thesis we use the Tully-Fisher relation (TFR), the correlation between a galaxy's luminosity...
We study the location of massive disc galaxies on the Tully-Fisher (TF) relation. Using a combinatio...
Context. Aims. We derive rotation curves from optical emission lines of 182 disc g...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
Aims. The relationship between baryonic and dark components in galaxies varies with the environment ...
Aims. We present spectroscopic observations of 182 disk galaxies (96 in the cluster and 86 in the fi...
We investigate the rich cluster Abell 2029 (z ~ 0.08) using optical imaging and long-slit spectral o...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
The Tully-Fisher Relation (TFR) links two fundamental properties of disk galaxies: their luminosity ...
In this thesis are presented the Tully-fisher (TF) relations for a sample of 99 galaxies within the ...
International audienceContext. Galaxies in dense environments are subject to interactions and mechan...
Galaxies form and evolve in different environments, arranged at large scales, in structures shaped b...
The research presented in this Ph.D thesis is mainly focused on the Tully– Fisher relation as a tool...
In this thesis we use the Tully-Fisher relation (TFR), the correlation between a galaxy's luminosity...
We study the location of massive disc galaxies on the Tully-Fisher (TF) relation. Using a combinatio...
Context. Aims. We derive rotation curves from optical emission lines of 182 disc g...
We have measured maximum rotation velocities (Vrot) for a sample of 111 emission-line galaxies with ...
Aims. The relationship between baryonic and dark components in galaxies varies with the environment ...
Aims. We present spectroscopic observations of 182 disk galaxies (96 in the cluster and 86 in the fi...
We investigate the rich cluster Abell 2029 (z ~ 0.08) using optical imaging and long-slit spectral o...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
The Tully-Fisher Relation (TFR) links two fundamental properties of disk galaxies: their luminosity ...
In this thesis are presented the Tully-fisher (TF) relations for a sample of 99 galaxies within the ...
International audienceContext. Galaxies in dense environments are subject to interactions and mechan...
Galaxies form and evolve in different environments, arranged at large scales, in structures shaped b...
The research presented in this Ph.D thesis is mainly focused on the Tully– Fisher relation as a tool...
In this thesis we use the Tully-Fisher relation (TFR), the correlation between a galaxy's luminosity...
We study the location of massive disc galaxies on the Tully-Fisher (TF) relation. Using a combinatio...