DEEP IMAGING WITH MILANKOVIĆ TELESCOPE: LINKING MERGER HISTORY TO KINEMATICS OF ELLIPTICAL GALAXIES
Ivana Ebrová, Michal Bílek, Ana Lalović, Mustafa K. Yıldız, Pierre-Alain Duc, Martin Mašek, Michael Prouza.
Publication
PUBLICATIONS OF THE ASTRONOMICAL OBSERVATORY OF BELGRADE104, Page 133-138, https://doi.org/10.69646/aob104p133
PROCEEDINGS of the XX Serbian Astronomical Conference, Belgrade, October 16 - 20, 2023, Edited by Jelena Petrović, Dušan Marčeta and Ana Lalović
Published by: Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia
Published: 15. 12. 2024.
Abstract
Abstract. Kinematical and morphological features observed in early-type galaxies provide valuable insights into the evolution of their hosts. We studied the origin of prolate rotation (i.e., rotation around the long axis) in Illustris large-scale cosmological hydrodynamical sim- ulations. We found that basically all the simulated massive prolate rotators were created in relatively recent major mergers of galaxies. Such mergers are expected to produce tidal features such as tails, shells, asymmetric stellar halos. We investigated deep optical images of prolate rotators, including newly obtained data from the Milankovic telescope (Astronomical Station Vidojevica), revealing signs of galaxy interaction in all of them. This correlation proves to be statistically very significant when compared with a general sample of early-type galaxies from the MATLAS deep imaging survey. In an ongoing project, we use the Milankovic telescope to assemble deep images of the complete sample of all known nearby massive prolate rotators. The most frequent tidal features among the prolate rotators happen to be shells. We developed methods to calculate the probable time of the merger from optical images. This will allow us to compare the merger history of the sample with predictions from Illustris. Our plan is to expand these methods to even larger samples of shell galaxies supplied by upcoming large surveys like LSST at Rubin Observatory. This will provide an unprecedented amount of statistically significant data on the recent merger history of our Universe and allow extensive investigation of the impact of mergers to a wide range of other astrophysical phenomena.