Where is the Cold Neutral Gas in the Hosts of High Redshift AGN?

S. J. Curran; M. T. Whiting; J. K. Webb

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arXiv · 0807.4983

Where is the Cold Neutral Gas in the Hosts of High Redshift AGN?

S. J. Curran·M. T. Whiting·J. K. Webb

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Abstract

Previous surveys for HI 21-cm absorption in z > 0.1 radio galaxies and quasars yield a 40% detection rate, which is attributed to unified schemes of active galactic nuclei (AGN). In this paradigm absorption is only witnessed in (close to) type-2 objects, where the central obscuration is viewed (nearly) edge-on and thus absorbs the rest frame 1420 MHz emission along our sight-line. However, we find this mix of detections and non-detections to only apply at low redshift (z < 1): From a sensitive survey of eight z > 3 radio sources we find no 21-cm absorption, indicating a low abundance of cold neutral gas in (the sight-lines searched in) these objects. Analysing the spectral energy distributions of these sources, we find that our high redshift selection introduces a bias where our sample consists exclusively of quasars with ultra-violet luminosities in excess of 10e23 W/Hz. This may suggest that we have selected a class of particularly UV bright type-1 objects. Whatever the cause, it must also be invoked to explain the non-detections in an equal number of z < 0.7 sources, where we find, for the first time, the same exclusive non-detections at > 10e23 W/Hz. These objects also turn out to be quasars and, from these exclusive high UV luminosity--21-cm non-detections, it is apparent that orientation effects alone cannot account for the mix of 21-cm detections and non-detections at any redshift.

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S. J. Curran, M. T. Whiting, J. K. Webb. 2008-07-31. Where is the Cold Neutral Gas in the Hosts of High Redshift AGN?. https://arxiv.org/abs/0807.4983

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