2011MNRAS.418.1787C


Query : 2011MNRAS.418.1787C

2011MNRAS.418.1787C - Mon. Not. R. Astron. Soc., 418, 1787-1795 (2011/December-2)

H I absorption towards nearby compact radio sources.

CHANDOLA Y., SIROTHIA S.K. and SAIKIA D.J.

Abstract (from CDS):

We present the results of H I absorption measurements towards a sample of nearby compact steep-spectrum (CSS) and gigahertz-peaked spectrum (GPS) radio sources, the Compact Radio sources at Low Redshift (CORALZ) sample, using the Giant Metrewave Radio Telescope (GMRT). We observed a sample of 18 sources and find seven new detections. These sources are of lower luminosity than earlier studies of CSS and GPS objects, and we investigate any dependence of H I absorption features on radio luminosity. Within the uncertainties, the detection rates and column densities are similar to the more luminous objects, with the GPS objects exhibiting a higher detection rate than for the CSS objects. The relative velocity of the blueshifted absorption features, which may be due to jet–cloud interactions, are within ∼ -250 km/s and do not appear to extend to values over 1000 km/s seen for the more luminous objects. This could be due to the weaker jets in these objects, but requires confirmation from observations of a larger sample of sources. There appears to be no evidence of any dependence of H I column density on either luminosity or redshift, but these new detections are consistent with the inverse relation between H I column density and projected linear size.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): galaxies: active - galaxies: evolution - galaxies: jets - galaxies: nuclei - radio lines: galaxies

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
2 ICRF J054236.1+495107 Sy1 05 42 36.13789710 +49 51 07.2337139   18.45 17.80 17.210   ~ 1573 1
3 QSO B0710+439 QSO 07 13 38.16413557 +43 49 17.2072102   20.7       ~ 256 0
4 NVSS J073328+560541 rG 07 33 28.6148 +56 05 41.730           ~ 32 1
5 2MASX J07393481+4954389 Bla 07 39 34.8468657150 +49 54 38.765761130           ~ 12 1
6 LEDA 2275964 Bla 08 31 39.8039 +46 08 00.775   18.94 18.07 13.6   ~ 38 1
7 7C 083313.50+441135.00 Sy2 08 36 37.8438240792 +44 01 09.576639372           ~ 26 1
8 6C 090251+464619 Bla 09 06 15.53979871 +46 36 19.0241852   16.80 16.08     ~ 63 1
9 LEDA 2269259 LIN 10 26 18.2613111266 +45 42 29.389879543           ~ 19 1
10 Z 212-30 LIN 10 37 19.3424977080 +43 35 15.305053488   14.6       ~ 91 1
11 6C 114716+554640 Bla 11 50 00.16487 +55 28 20.8780       14.3   ~ 29 1
12 NVSS J120902+411559 rG 12 09 02.7905671200 +41 15 59.305654152           ~ 16 1
13 6C 121638+484640 Bla 12 19 06.41475008 +48 29 56.1647529   21.22 20.49 19.90   ~ 146 1
14 6C 122535+365318 QSO 12 27 58.72552577 +36 35 11.8265176   21.5 21.5     ~ 139 1
15 ICRF J131739.1+411545 Bla 13 17 39.1954 +41 15 45.621           ~ 54 1
16 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
17 2MASX J14005162+5216068 LIN 14 00 51.5814702864 +52 16 06.473503164           ~ 21 1
18 87GB 140732.1+361738 Sy1 14 09 42.4485402456 +36 04 15.887047296           ~ 25 1
19 6C 143339+510410 LIN 14 35 21.6699085551 +50 51 22.922806306           ~ 24 1
20 Z 193-16 rG 15 08 05.69280 +34 23 23.3376   15.6       ~ 50 1
21 4C 52.37 Sy1 16 02 46.3870735776 +52 43 58.675644984   18.50 17.76     ~ 45 1
22 4C 40.34 BLL 16 11 48.5301162024 +40 40 20.955442404           ~ 26 1
23 6C 161147+342017 Bla 16 13 41.06424322 +34 12 47.9088535   17.98 17.46 17.07   ~ 673 1
24 ICRF J163433.8+624535 Sy2 16 34 33.80623119 +62 45 35.8960467   21.06 20.61     ~ 220 1
25 6C 170204+454510 Sy1 17 03 30.3824218008 +45 40 47.166180564   16.0       ~ 170 2
26 2MASX J17185436+5441486 Sy2 17 18 54.4002 +54 41 48.289           ~ 84 1

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