Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-06-06
Mon.Not.Roy.Astron.Soc.379:1546-1556,2007
Astronomy and Astrophysics
Astrophysics
13 pages, 5 figures, accepted for publication in MNRAS
Scientific paper
10.1111/j.1365-2966.2007.12062.x
We report a definitive confirmation of a large-scale structure around the super rich cluster CL0016+1609 at z=0.55. We made spectroscopic follow-up observations with FOCAS on Subaru along the large filamentary structure identified in our previous photometric studies. We have confirmed the physical connection of the huge filament extending over 20 Mpc in the N-S direction, and another filament extending from the main cluster to the East. Based on a simple energy argument, we show that it is likely that most of the clumps are bound to the main CL0016 cluster. This structure is surely one of the most prominent confirmed structures ever identified in the distant Universe, which then serves as an ideal laboratory to examine the environmental variation of galaxy properties. We draw star formation histories of galaxies from the composite spectra of red galaxies in field, group, and cluster environments. Combining the results from our previous studies, we find that red galaxies in groups at z~0.8 and red field galaxies at z~0.5 show strong Hd absorption lines for their D4000 indices. These are the environments in which we observed the on-going build-up of the colour-magnitude relation in our previous photometric analyses. The strong Hd absorption lines imply that their star formation is truncated on a relatively short time scale. We suggest that a galaxy-galaxy interaction is the most likely physical driver of the truncation of star formation and thus responsible for the build-up of the colour-magnitude relation since z~1. (Abridged)
Hoshi Takako
Kashikawa Nobunari
Kodama Tadayuki
Tanaka Masayuki
No associations
LandOfFree
A Huge Filamentary Structure at z=0.55 and Star Formation Histories of Galaxies at z<1 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Huge Filamentary Structure at z=0.55 and Star Formation Histories of Galaxies at z<1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Huge Filamentary Structure at z=0.55 and Star Formation Histories of Galaxies at z<1 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-356751