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.
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.
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