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Spectroscopy of Ultra--Steep Spectrum Radio Sources: A Sample of z>2 Radio Galaxies | H.J.A. Röttgering
; R. van Ojik
; G.K. Miley
; K.C. Chambers
; W.J.M. van Breugel
; S. de Koff
; | Date: |
12 Aug 1996 | Subject: | astro-ph | Abstract: | 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 ($alpha < -1$) 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, Ly$alpha$ is almost always the dominant emission line, with a rest frame equivalent width ranging from $sim100$ AA to more than 1000 AA. The equivalent widths of the most important emission lines (Ly$alpha$, 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 Ly$alpha$ 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 Ly$alpha$ emission line may be | Source: | arXiv, astro-ph/9608063 | Services: | Forum | Review | PDF | Favorites |
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