Bibcode
Pintos-Castro, I.; Pović, M.; Sánchez-Portal, M.; Cepa, J.; Altieri, B.; Bongiovanni, Á.; Duc, P. A.; Ederoclite, A.; Oteo, I.; Pérez García, A. M.; Pérez Martínez, R.; Polednikova, J.; Ramón-Pérez, M.; Temporin, S.
Bibliographical reference
Astronomy and Astrophysics, Volume 592, id.A108, 19 pp.
Advertised on:
8
2016
Journal
Citations
7
Refereed citations
5
Description
Studying the evolution of the morphological distribution of galaxies in
different environments can provide important information about the
effects of the environment and the physical mechanisms responsible for
the morphological transformations. As part of a complete analysis of the
young cluster RXJ 1257+4738 at z ~ 0.9, in this work we study the
morphological properties of its galaxies. We used non-parametric methods
of morphological classification, as implemented in the galSVM code. The
classification with the applied method was possible even using
ground-based observations, as the r'-band imaging from OSIRIS/GTC. We
defined very conservative probability limits, taking into account the
probability errors, to obtain a trustworthy classification. In this way
we were able to classify ~30% of all cluster members and to separate
between late-type (LT) and early-type (ET) galaxies. Additionally, when
analysing the colour-magnitude diagram, we observed a significant
population of blue ET galaxies among the classified ones. We discussed
possible explanations for finding this population. Moreover, we studied
different physical properties of LT, ET, and blue ET galaxies. They turn
out to be comparable, with the exception of the stellar mass that shows
that the red ET population is more massive. We also analysed the
morphology-density and morphology-radius relations observing that, only
when considering the morphological separation between ET and LT
galaxies, a mild classical behaviour is obtained. RXJ 1257+4738 is a
young galaxy cluster, showing a clumpy structure, which is still in the
process of formation, and which could explain the lack of some of the
standard morphological relations. This makes this cluster a very
attractive case for obtaining higher resolution data and for studying
the morphological properties of the entire cluster in more detail and
their relation to the environment.
The catalogues are only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/592/A108