Bibcode
Barrera-Ballesteros, J. K.; García-Lorenzo, B.; Falcón-Barroso, J.; van de Ven, G.; Lyubenova, M.; Wild, V.; Méndez-Abreu, J.; Sánchez, S. F.; Marquez, I.; Masegosa, J.; Monreal-Ibero, A.; Ziegler, B.; del Olmo, A.; Verdes-Montenegro, L.; García-Benito, R.; Husemann, B.; Mast, D.; Kehrig, C.; Iglesias-Paramo, J.; Marino, R. A.; Aguerri, J. A. L.; Walcher, C. J.; Vílchez, J. M.; Bomans, D. J.; Cortijo-Ferrero, C.; González Delgado, R. M.; Bland-Hawthorn, J.; McIntosh, D. H.; Bekeraitė, S.
Bibliographical reference
Astronomy and Astrophysics, Volume 582, id.A21, 50 pp.
Advertised on:
10
2015
Journal
Citations
96
Refereed citations
91
Description
We present spatially resolved stellar and/or ionized gas kinematic
properties for a sample of 103 interacting galaxies, tracing all merger
stages: close companions, pairs with morphological signatures of
interaction, and coalesced merger remnants. In order to distinguish
kinematic properties caused by a merger event from those driven by
internal processes, we compare our galaxies with a control sample of 80
non-interacting galaxies. We measure for both the stellar and the
ionized gas components the major (projected) kinematic position angles
(PAkin, approaching and receding) directly from the velocity
distributions with no assumptions on the internal motions. This method
also allow us to derive the deviations of the kinematic PAs from a
straight line (δPAkin). We find that around half of the
interacting objects show morpho-kinematic PA misalignments that cannot
be found in the control sample. In particular, we observe those
misalignments in galaxies with morphological signatures of interaction.
On the other hand, thelevel of alignment between the approaching and
receding sides for both samples is similar, with most of the galaxies
displaying small misalignments. Radial deviations of the kinematic PA
orientation from a straight line in the stellar component measured by
δPAkin are large for both samples. However, for a large
fraction of interacting galaxies the ionized gas δPAkin
is larger than the typical values derived from isolated galaxies (48%),
indicating that this parameter is a good indicator to trace the impact
of interaction and mergers in the internal motions of galaxies. By
comparing the stellar and ionized gas kinematic PA, we find that 42%
(28/66) of the interacting galaxies have misalignments larger than
16°, compared to 10% from the control sample. Our results show the
impact of interactions in the motion of stellar and ionized gas as well
as the wide the variety of their spatially resolved kinematic
distributions. This study also provides a local Universe benchmark for
kinematic studies in merging galaxies at high redshift.
Appendices are available in electronic form at http://www.aanda.org
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