Catalog Service: Optical view of Abell 85 filament region
Description
We present an optical investigation of the Abell 85 cluster filament (z=0.055) previously interpreted in X-rays as groups falling on to the main cluster. We compare the distribution of galaxies with the X-ray filament, and investigate the galaxy luminosity functions in several bands and in several regions. We search for galaxies where star formation may have been triggered by interactions with intracluster gas or tidal pressure due to the cluster potential when entering the cluster.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2009 Feb 14 06:25:50ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/A+A/489/11/tablea4 (Broad band magnitudes of the 101 objects detected in H{alpha})
VERB=1
VERB=3
Cone search capability for table J/A+A/489/11/tablea5 (Broad band magnitudes of the 6 galaxies with H{alpha} emission in their SDSS spectra but not detected in our narrow band filter due to its wavelength cut)
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