1996/08/12 by H. J. A. Röttgering, R. van Ojik, Röttgering, H. J. A. +9
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9608063
Accepted for publication in Astronomy and Astrophysics
arxiv created 1996/08/12 · arxiv updated 2009/12/01
We present spectroscopic observations for 64 radio galaxies having ultra steep radio spectra. Twenty-nine objects have redshifts z>2, the largest redshifts being almost 4. Our ultra steep spectrum (USS) criterion (α< -1) has proven to be the most efficient way of finding distant radio galaxies. We find that even among the USS sources, there is a strong statistical correlation between the spectral index and redshift. The most distant radio galaxies within the USS sample have the steepest radio spectra. In our sample there are 3 radio galaxies at z>3 compared with 26 at 2 < z < 3. However, the present data do not allow us to decide whether there is a decrease in co-moving source density at the highest redshifts. We have analyzed the spectra of the 30 objects with the highest redshifts (z>1.9). For these high redshift radio galaxies, Lyα is almost always the dominant emission line, with a rest frame equivalent width ranging from ∼100 Å to more than 1000 Å. The equivalent widths of the most important emission lines (Lyα, C \small IV, He \small II, C \small III]) are found to correlate strongly with each other. The large rest frame equivalent widths and the correlation between the equivalent widths of the emission lines, confirm that photoionization by a central continuum source is most likely the dominant ionization mechanism. There are significant velocity differences between the various emission lines of our high redshift radio galaxies; in particular the Lyα line is shifted with respect to the higher ionization lines. Velocity shifts range from 100 to almost 1000 km s-1 in some cases. Simulations show that the effects of associated H \small I absorption on the Lyα emission line may be