Photometry of the 3C324 Cluster and Line/off Line of the Radio Galaxy

Details Photometry of the 3C324 Cluster and Line/off Line of the Radio Galaxy Photometry of the 3C324 Cluster and Line/off Line of the Radio Galaxy

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7224s&link_type=abstract

HST Proposal ID #7224

Mathematics

Logic

Hst Proposal Id #7224 Clusters Of Galaxies

Scientific paper

Spatially-resolved IR photometry of the aligned radio galaxy 3C 324 {z=1.206} and its surrounding cluster of E galaxies should be an important step in our understanding of the alignment effect in powerful radio galaxies and in our study of the passive evolution of the oldest systems. Ground-based K-band imaging by Dickinson and collaborators has located a surrounding cluster of fairly uniform profile, very red galaxies: with NICMOS we intend to examine the galaxies' morphological uniformity, absolute H-band fluxes, and effective radii needed to evaluate a Tolman-like cosmological test. Much of the integration time will utilize a filter selected to transmit the redshifted H-alpha line. The collaborators on this investigation are Mark Dickinson {Postdoc, STScI} and Andrew Bunker {NICMOS Postdoc, UC Berkeley}.

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