1996/01/11 by C A Jackson, Jackson, C A
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9601051
2 pages, 1 postscript figure, uses crckapb.sty style file; Proceedings of IAU 175, Bologna 1995, Kluwer Academic Press
arxiv created 1996/01/11 · arxiv updated 2009/12/01
Previous analyses of the space densities of extragalactic radio sources have proceeded on the assumption of two populations: flat-spectrum and steep-spectrum objects, compact and extended in radio structure respectively. It is now generally believed that anisotropic radiation and relativistic beaming effects mean that the steep-spectrum objects are the flat-spectrum objects viewed side-on. The implication is that all previous space density analyses start from the wrong basic premise. There are two unifying paradigms extant for the powerful radio sources, one relating flat-spectrum QSOs and the steep-spectrum FRII sources, the other the BL Lac objects with FRI sources. Our new investigation of space distribution and luminosity functions takes these two populations as a starting point in a new parametric analysis of space densities. The present paper describes the datasets, methodology and first results.