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Table 6

Data from HNC 1-0 observations.

Galaxy I(HNC) 1-0a SνΔv Δv Telescope ηmb θmb T scalea References
[K km s-1] [Jy km s-1] [km s-1] [′′]

Arp 220 0.95 ± 0.2 26  ±  6 ... SEST 15 m 0.75 55 (1)
Circinus 1.99 ± 0.1 55  ±  3 280 SEST 15 m 0.75 55 (2)
IC 342 9.2 ± 0.7 48  ±  4 47 IRAM 30 m 0.8 25 (3)
IC 694 0.75 ± 0.2 15  ±  4 300-400 OSO 20 m 0.59 42 (1)
IC 860 0.70 ± 0.04 4.6  ±  0.3 230 IRAM 30 m 0.80 28 (2)
I17208 1.12 ± 0.06 7.4  ±  0.4 350 IRAM 30 m 0.80 28 (2)
M82 7.3 ± 0.6 31  ±  3 129 IRAM 30 m 0.64 25 Tmb (4)
Maffei 2 7.3 ± 0.8 31  ±  3 91, 50 IRAM 30 m 0.64 25 Tmb (4)
NGC 34  < 0.44  < 12 ... SEST 15 m 0.75 55 (2)
NGC 253 50.0 ± 2.8 210  ±  12 72, 136 IRAM 30 m 0.64 25 Tmb (4)
NGC 613  < 0.24  < 6.5 ... SEST 15 m 0.75 55 (2)
NGC 1056  < 0.17  < 1.1 ... IRAM 30 m 0.80 28 (2)
NGC 1068 3.2 ± 0.5 65  ±  10 260 SEST 15 m 0.75 55 Tmb (5)
NGC 1068 11.4 ± 0.7 48  ±  3 232 IRAM 30 m 0.64 25 Tmb (4)
NGC 1365 4.7 ± 0.6 96  ±  12 150 SEST 15 m 0.75 55 Tmb (5)
NGC 1377  < 0.15  < 0.99 ... IRAM 30 m 0.80 28 (2)
NGC 1614  < 0.38  < 10 ... SEST 15 m 0.75 55 (2)
NGC 1808 1.2 ± 0.1 33  ±  3 300 SEST 15 m 0.75 55 (1)
NGC 2146 1.6 ± 0.3 6.7  ±  1.3 237 IRAM 30 m 0.64 25 Tmb (4)
NGC 2623 0.6 ± 0.15 12  ±  3 500-600 OSO 20 m 0.59 42 (1)
NGC 3079 2.9 ± 0.5 15  ±  3 380 IRAM 30 m 0.80 28 Tmb (5)
NGC 3079 6.9 ± 1.0 29  ±  4 545 IRAM 30 m 0.64 25 Tmb (4)
NGC 3256 0.6 ± 0.05 16  ±  1 250 SEST 15 m 0.75 55 (1)
NGC 3690 ... ... ... ... ... N/Aa
NGC 4418 1.24 ± 0.12 7.9  ±  0.8 156 IRAM 30 m 0.77 27 (6)
NGC 4945 8.6 ± 0.2 230  ±  5 290 SEST 15 m 0.75 55 (2)
NGC 5135  < 0.13  < 3.5 ... SEST 15 m 0.75 55 (2)
NGC 6946 4.0 ± 0.3 17  ±  1 138 IRAM 30 m 0.64 25 Tmb (4)
NGC 7130 0.4 ± 0.05 11  ±  1 ... SEST 15 m 0.75 55 (1)
UGC 5101 1.24 ± 0.1 8.2  ±  0.7 500 IRAM 30 m 0.80 28 (2)

References. (1) Aalto et al. (2002); (2) This work; (3) Henkel et al. (1988); (4) Hüttemeister et al. (1995); (5) Pérez-Beaupuits et al. (2007); (6) Aalto et al. (2007).

Notes. 

(a)

The temperature scale of the integrated intensities are given in the T scale column. Upper limits are 2σ calculated from the rms of the noise surrounding the line for our data. For our data, errors are given in 1σ and calculated from the rms. Since many articles lack information about sizes of errors and methods used when calculating the errors, most errors are given as printed in the respective article. However, if the size of the error is clearly written, it has been recalculated to 1σ.

(b)

No HNC data were found in the literature for this object.

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