2012MNRAS.421..651S


Query : 2012MNRAS.421..651S

2012MNRAS.421..651S - Mon. Not. R. Astron. Soc., 421, 651-665 (2012/March-3)

Search for cold gas in z > 2 damped Lyα systems: 21-cm and H2 absorption.

SRIANAND R., GUPTA N., PETITJEAN P., NOTERDAEME P., LEDOUX C., SALTER C.J. and SAIKIA D.J.

Abstract (from CDS):

We present the results of a systematic Green Bank Telescope and Giant Metrewave Radio Telescope survey for 21-cm absorption in a sample of 10 damped Lyman α systems (DLAs) at 2 ≤ zabs ≤ 3.4. Analysis of L-band very long baseline array images of the background QSOs are also presented. We detect 21-cm absorption in only one DLA (at zabs= 3.1745 towards J1337+3152). Thus the detection rate of 21-cm absorption is ∼ 10 per cent when no limit on the integrated optical depth (∫τ(v)dv) is imposed and ∼ 13 per cent for a 3σ limit of 0.4 km/s. Combining our data with the data from the literature (a sample of 28 DLAs) and assuming the measured core fraction at milliarcsecond scale to represent the gas covering factor, we find that the H I gas in DLAs at z ≥ 2 is predominantly constituted by a warm neutral medium. The detection rate of 21-cm absorption seems to be higher for systems with higher N(H I) or metallicity. However, no clear correlation is found between the integrated 21-cm optical depth (or the spin temperature, TS) and either N(H I), metallicity or velocity spread of the low-ionization species. There are 13 DLAs in our sample for which high-resolution optical spectra covering the expected wavelength range of H2 absorption are available. We report the detection of H2 molecules in the zabs= 3.3871 21-cm absorber towards J0203+1134 (PKS 0201+113). In eight cases, neither H2(with molecular fraction f(H2) ≤ 10–6) nor 21-cm absorption (with TS/fc ≥ 700 K) is detected. The lack of 21-cm and H2 absorption in these systems can be explained if most of the H I in these DLAs originates from low-density high-temperature gas. In one case we have a DLA with 21-cm absorption not showing H2absorption. In two cases, both species are detected but do not originate from the same velocity component. In the remaining two cases 21-cm absorption is not detected despite the presence of H2 with evidence for the presence of cold gas. All this is consistent with the idea that the H2components seen in DLAs are compact (with sizes of ≤ 15 pc) and contain only a small fraction (i.e. typically ≤ 10 per cent) of the total N(H I) measured in the DLAs. This implies that the molecular fractions f(H2) reported from the H2 surveys should be considered as conservative lower limits for the H2components.

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): galaxies: ISM - quasars: absorption lines

Simbad objects: 48

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Number of rows : 48
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 QSO B0201+113 QSO 02 03 46.65705710 +11 34 45.4094619   19.5 19.5 19.41   ~ 204 1
2 3C 82 QSO 03 14 43.6 +43 14 05     21.0     ~ 51 2
3 QSO B0335-122 QSO 03 37 55.4513467728 -12 04 04.551994488   21.018 20.110 20.199   ~ 78 1
4 QSO B0336-017 QSO 03 39 00.98616588 -01 33 17.6076051   20.1 19.1 18.8   ~ 117 2
5 QSO J0407-4410 QSO 04 07 18.0880236912 -44 10 13.983623724   17.6 17.6     ~ 99 0
6 QSO B0405-331 QSO 04 07 33.91372765 -33 03 46.3581465   19.33   19.77   ~ 61 1
7 QSO B0432-440 QSO 04 34 03.2139497184 -43 55 47.757093672   19.8 19.60 19.7   ~ 39 0
8 QSO B0438-43 QSO 04 40 17.17997576 -43 33 08.6043290   19.31 19.5 18.2   ~ 287 2
9 4C -02.19 QSO 05 01 12.80988538 -01 59 14.2564557   19.1 18.06 19.04   ~ 585 1
10 QSO B0528-2505 QSO 05 30 07.9627395840 -25 03 29.900044512   18.17 17.34 17.7   ~ 420 0
11 QSO B0537-286 Bla 05 39 54.28147904 -28 39 55.9481236   19.70 20.0 18.789   ~ 290 1
12 7C 055201.39+394824.00 Bla 05 55 30.80561419 +39 48 49.1649683     18.30 17.5   ~ 505 2
13 ICRF J073256.2+254838 QSO 07 32 56.27526878 +25 48 38.7956244   18.75 18.46 19.08   ~ 41 1
14 [VV2006] J073320.5+272103 QSO 07 33 20.4880276656 +27 21 03.472646508   19.90 19.60     ~ 42 1
15 7C 075105.29+483138.00 BLL 07 54 45.6705975216 +48 23 50.749279404   17.97 17.55 16.4   ~ 76 1
16 QSO J0801+4725 QSO 08 01 37.6870069320 +47 25 28.171357680   20.71 20.00     ~ 38 1
17 7C 080458.39+495918.00 QSO 08 08 39.66628970 +49 50 36.5304041   19.55 19.18 18.34   ~ 362 2
18 QSO J0816+4823 QSO 08 16 18.9961577208 +48 23 28.468011444   20.77 19.89     ~ 47 1
19 SDSS J083910.89+200207.3 QSO 08 39 10.8994134984 +20 02 07.334544156   20.46 20.22     ~ 31 1
20 QSO B0839+187 Bla 08 42 05.0940565824 +18 35 40.988568300   16.63 16.36 16.56   ~ 185 2
21 SDSS J085257.12+243103.1 QSO 08 52 57.1213050144 +24 31 03.182860416   21.02 20.28     ~ 37 1
22 ICRF J085657.2+211143 QSO 08 56 57.24476663 +21 11 43.6582291   20.04 19.82 19.92   ~ 57 1
23 QSO B0913+003 BLL 09 15 51.69513598 +00 07 13.3089688   21.7 21.70 19.5   ~ 41 1
24 ICRF J092703.0+390220 Sy1 09 27 03.01394144 +39 02 20.8518067   17.17 17.00 16.486   ~ 1001 1
25 6C 101357+613120 QSO 10 17 25.88756462 +61 16 27.4965040   18.74 18.44 17.87   ~ 93 1
26 7C 102826.00+603558.00 QSO 10 31 44.7563408352 +60 20 30.365432664   18.55 18.29 18.2   ~ 80 1
27 6C 122116+505501 BLL 12 23 43.1690899704 +50 37 53.412268908   18.62 18.05     ~ 50 1
28 6C 122527+494833 QSO 12 27 55.7276 +49 32 56.042     20.3 19.82   ~ 40 1
29 ICRF J123413.3+475351 Sy1 12 34 13.3306496760 +47 53 51.237796812   17.62 17.31 16.8   ~ 83 1
30 LBQS 1232+0815 QSO 12 34 37.5514444464 +07 58 43.367750796     18.4     ~ 125 0
31 [VV2006] J123717.4+470807 QSO 12 37 17.4391451928 +47 08 07.025601048   19.51 19.12     ~ 35 1
32 6C 123945+373654 QSO 12 42 09.81238457 +37 20 05.6921765   20.60 19.82     ~ 76 1
33 6C 124026+380741 QSO 12 42 51.36906848 +37 51 00.0252818   18.86 18.46 18.79   ~ 92 1
34 7C 132734.79+320943.00 BLL 13 29 52.86491586 +31 54 11.0544317   20.96 20.23 19.77   ~ 63 1
35 QSO J1337+3152 QSO 13 37 24.6964232832 +31 52 54.575696928   19.40 19.01     ~ 52 1
36 QSO J1356-1101 QSO 13 56 46.8321231864 -11 01 29.227444572   19.0 19.20 17.7   ~ 52 1
37 QSO B1354-174 QSO 13 57 06.07420758 -17 44 01.9049954   19 19 18   ~ 91 1
38 QSO B1402+044 QSO 14 05 01.11981857 +04 15 35.8188818   19.86 19.53 19.22   ~ 193 1
39 [VV2006] J140653.9+343336 QSO 14 06 53.8472771496 +34 33 37.310323356   19.17 18.84 18.02   ~ 76 1
40 [VV2006] J141318.9+450523 QSO 14 13 18.8641 +45 05 23.012   20.70 19.98 19.27   ~ 47 1
41 NVSS J141604+344436 Rad 14 16 04.18619489 +34 44 36.4264542           ~ 93 1
42 4C 46.29 QSO 14 17 08.1615256776 +46 07 05.449251216   18.13 17.99     ~ 99 1
43 QSO B1418-064 QSO 14 21 07.75560722 -06 43 56.3557864   20.4 18.50 19.1   ~ 74 0
44 6C 142744+541929 QSO 14 29 21.87879031 +54 06 11.1228062   20.73 20.39 20.5   ~ 93 1
45 6C 143400+544902 QSO 14 35 33.7785 +54 35 59.308   21.67 20.87     ~ 40 1
46 7C 175844.60+384828.00 QSO 18 00 24.76536016 +38 48 30.6974570   17.8 17.98 17.04   ~ 151 1
47 3C 454.3 Bla 22 53 57.7480438728 +16 08 53.561508864   16.57 16.10 15.22   ~ 2847 2
48 QSO B2342+3417 QSO 23 44 51.2526572424 +34 33 48.696770052     19.1     ~ 64 1

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