We used FORS2 in MXU mode to mimic a coarse 'IFU' in order to measure the 3D large-scale kinematics around the central Hydra I cluster galaxy NGC 3311. Our data show that the velocity dispersion field varies as a function of radius and azimuthal angle and violates point symmetry. Also, the velocity field shows similar dependence, hence the stellar halo of NGC 3311 is a dynamically young structure. The kinematic irregularities coincide in position with a displaced diffuse halo North-East of NGC 3311 and with tidal features of a group of disrupting dwarf galaxies. This suggests that the superposition of different velocity components is responsible for the kinematic substructure in the Hydra I cluster core.
@article{arxiv.1410.0695,
title = {A 3D view of the Hydra I galaxy cluster core - I. Kinematic substructures},
author = {Michael Hilker and Carlos Eduardo Barbosa and Tom Richtler and Lodovico Coccato and Magda Arnaboldi and Claudia Mendes de Oliveira},
journal= {arXiv preprint arXiv:1410.0695},
year = {2015}
}
Comments
2 pages, highlight talk in the IAU Symposium 309: "Galaxy in 3D across the Universe", Vienna, 7-11 July 2014; B. L. Ziegler, F. Combes, H. Dannerbauer, M. Verdugo, Eds. (Cambridge: Cambridge Univ. Press), in press