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The Nature Of Ultraluminous Iras Galaxies
[chapter]
1999
Galaxy Interactions at Low and High Redshift
We present the results of a continuing programme to investigate the properties of the Ultraluminous IRAS Galaxies (ULIRGs) in a large sample selected from the IRAS Faint Source Catalogue and identified with the APM galaxy catalogue (for details of the survey selection and initial results see Clements et al. 1996, MNRAS, 279, 459). Observations now include optical imaging for a complete subsample to BJ = 19.5 (Clements et al. 1996, MNRAS, 279, 477) and near-IR imaging for a complete subsample to
doi:10.1007/978-94-011-4665-4_86
fatcat:2oy2fthisvgodbrjcwzrodsfra