C.D.S. - SIMBAD4 rel 1.7 - 2019.11.19CET10:05:59

2014A&A...569A..35G - Astronomy and Astrophysics, volume 569A, 35-35 (2014/9-1)

Probing the gas content of radio galaxies through HI absorption stacking.


Abstract (from CDS):

Using the Westerbork Synthesis Radio Telescope, we carried out shallow HI absorption observations of a flux-selected (S1.4GHz>50mJy) sample of 93 radio active galactic nuclei (AGN), which have available SDSS (Sloan Digital Sky Survey) redshifts between 0.02<z<0.23. Our main goal is to study the gas properties of radio sources down to S1.4GHz flux densities not systematically explored before using, for the first time, stacking of absorption spectra of extragalactic HI. Despite the shallow observations, we obtained a direct detection rate of ∼29%, comparable with deeper studies of radio galaxies. Furthermore, detections are found at every S1.4GHz flux level, showing that HI absorption detections are not biased toward brighter sources. The stacked profiles of detections and non-detections reveal a clear dichotomy in the presence of HI, with the 27 detections showing an average peak τ=0.02 corresponding to N(HI)~(7.4±0.2)x1018(Tspin/cf)/cm2, while the 66 non-detections remain undetected upon stacking with a peak optical depth upper limit τ< 0.002 corresponding to N(HI)<(2.26±0.06)x1017(Tspin/cf)/cm2 (using a FWHM of 62km/s, derived from the mean width of the detections). Separating the sample into compact and extended radio sources increases the detection rate, optical depth, and FWHM for the compact sample. The dichotomy for the stacked profiles of detections and non-detections still holds between these two groups of objects. We argue that orientation effects connected to a disk-like distribution of the HI can be partly responsible for the dichotomy that we see in our sample. However, orientation effects alone cannot explain all the observational results, and some of our galaxies must be genuinely depleted of cold gas. A fraction of the compact sources in the sample are confirmed by previous studies as likely young radio sources (compact steep spectrum and gigahertz peaked spectrum sources). These show an even higher detection rate of 55%. Along with their high integrated optical depth and wider profile, this reinforces the idea that young radio AGN are embedded in a medium that is rich in atomic gas. Part of our motivation is to probe for the presence of faint HI outflows at low optical depth using stacking. However, the stacked profiles do not reveal any significant blueshifted wing. We are currently collecting more data to investigate the presence of outflows. The results presented in this paper are particularly relevant for future surveys in two ways. The lack of bias toward bright sources is encouraging for the search for HI in sources with even lower radio fluxes planned by such surveys. The results also represent a reference point when searching for HI absorption at higher redshifts.

Abstract Copyright:

Journal keyword(s): galaxies: active - ISM: jets and outflows - radio lines: galaxies

Simbad objects: 6

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Number of rows : 6

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
1 4C 12.05 BLL 00 38 18.1071 +12 27 32.468   20.0       ~ 38 2
2 NGC 315 LIN 00 57 48.88335 +30 21 08.8122 12.80 12.20 11.16 11.26   ~ 683 2
3 UGC 8782 LIN 13 52 17.765 +31 26 46.10   16.10 15.10     ~ 417 3
4 IC 1065 Sy2 14 49 21.5921149894 +63 16 13.816373757   17.30 16.39     ~ 330 1
5 QSO B1946+708 Bla 19 45 53.51992731 +70 55 48.7321708   18.726 16.70 17.199   ~ 124 2
6 ICRF J235509.4+495008 Sy2 23 55 09.45814510 +49 50 08.3395036   21.101   18.400   ~ 243 1

    Equat.    Gal    SGal    Ecl

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