We have examined the orientations of early-type galaxies in the Coma cluster to see whether the well-established tendency for brightest cluster galaxies to share the same major axis orientation as their host cluster also extends to the rest of the galaxy population. We find no evidence of any preferential orientations of galaxies within Coma or its surroundings. The implications of this result for theories of the formation of clusters and galaxies (particularly the first-ranked members) are discussed
Coma is frequently used as the archetype z ∼ 0 galaxy cluster to compare higher redshift work agains...
In this work, we combine ellipticity and major axis position angle measurements from the Sloan Digit...
The mean redshift of the core of the Coma cluster - cz = 6953 km s^{-1} and its dispersion \sigma=94...
Accepted in A&AWe have then searched for preferential orientations of faint galaxies in the Coma clu...
Analysis of photometry data of the Coma Cluster galaxies shows a prominent effect of galaxy alignmen...
For a sample of 122 rich Abell clusters the authors find a strong correlation of the position angle ...
We use galaxy groups selected from the Sloan Digital Sky Survey to examine the alignment between the...
We present an analysis of the spatial orientations of 323 galaxies in the cluster Abell 3558. Our ai...
It is known observationally that the major axes of galaxy clusters and their brightest cluster galax...
We present a quantitative morphological analysis of 187 galaxies in a region covering the centr...
We present a quantitative morphological analysis of 187 galaxies in a region covering the central 0....
We analysed some properties of galaxies structures based on the PF catalog of galaxy structures (Pan...
Coma is frequently used as the archetype z ∼ 0 galaxy cluster to compare higher redshift work agains...
In this work, we combine ellipticity and major axis position angle measurements from the Sloan Digit...
The mean redshift of the core of the Coma cluster - cz = 6953 km s^{-1} and its dispersion \sigma=94...
Accepted in A&AWe have then searched for preferential orientations of faint galaxies in the Coma clu...
Analysis of photometry data of the Coma Cluster galaxies shows a prominent effect of galaxy alignmen...
For a sample of 122 rich Abell clusters the authors find a strong correlation of the position angle ...
We use galaxy groups selected from the Sloan Digital Sky Survey to examine the alignment between the...
We present an analysis of the spatial orientations of 323 galaxies in the cluster Abell 3558. Our ai...
It is known observationally that the major axes of galaxy clusters and their brightest cluster galax...
We present a quantitative morphological analysis of 187 galaxies in a region covering the centr...
We present a quantitative morphological analysis of 187 galaxies in a region covering the central 0....
We analysed some properties of galaxies structures based on the PF catalog of galaxy structures (Pan...
Coma is frequently used as the archetype z ∼ 0 galaxy cluster to compare higher redshift work agains...
In this work, we combine ellipticity and major axis position angle measurements from the Sloan Digit...
The mean redshift of the core of the Coma cluster - cz = 6953 km s^{-1} and its dispersion \sigma=94...