Panoramic and Multi-Wavelength Study of the Distant Cluster RXJ1716 at z= 0.81

Details Panoramic and Multi-Wavelength Study of the Distant Cluster RXJ1716 at z= 0.81 Panoramic and Multi-Wavelength Study of the Distant Cluster RXJ1716 at z= 0.81

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..399..361k&link_type=abstract

Panoramic Views of Galaxy Formation and Evolution ASP Conference Series, Vol. 399, proceedings of the conference held 11-16 Dece

Astronomy and Astrophysics

Astronomy

Scientific paper

We study galaxies in and around the distant cluster RXJ1716 (z=0.81) using deep and panoramic optical to mid-infrared imaging data obtained with Suprime-Cam on Subaru and IRC on the AKARI satellite. We find that the cluster member candidates detected at 15~μm are preferentially found in medium-density environments such as subclumps or filaments around the cluster. This suggests that the star-formation activity in galaxies is enhanced in those regions due to some environmental effects specific to such medium-density environments. This is before it is completely truncated as a consequence of quick gas consumption and/or removal.

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