Open AccessDrag‐gravity torques on galaxies in clusters: radial small‐scale alignment effects
Author(s) -
GonzálezSánchez Alejandro,
Teodoro Luís F. A.
Publication year - 2010
Publication title -
monthly notices of the royal astronomical society: letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.067
H-Index - 122
eISSN - 1745-3933
pISSN - 1745-3925
DOI - 10.1111/j.1745-3933.2010.00824.x
Subject(s) - physics , astrophysics , cluster (spacecraft) , galaxy cluster , galaxy , brightest cluster galaxy , computer science , programming language
We calculate the torque on galaxies in clusters due to gravity and to dynamical friction forces in order to study the possible origin of small‐scale alignment effects as the result of interactions with their environment. The equation of motion for the position angle of a galaxy is derived by using a simple model. We find that weak radial alignment effects can be produced by this mechanism involving only the most massive galaxies. We also introduce a dependence on the cluster eccentricity to our equations in order to explore the alignment of galaxies with the cluster's major axis. We find that in the inner regions of high eccentricity clusters, alignments of massive galaxies with the cluster's major axis dominate over the radial ones. This mechanism could account for the observed alignment effects of the most massive galaxies with the major axis of their host cluster. Our results suggest that dynamical friction is a viable generator of alignment only for the most massive cluster galaxies. For the observed alignments of normal galaxies a primordial origin has to be explored.