Table 2
Measured line parameters.
| Source | Line | Vhelio | ΔV | Tl | Tc | ||
| km s-1 | km s-1 | mK | mK | ||||
|
|
|||||||
| NGC 4945 (n) | H2O | +645(1) | 80(1) | –271(3) | 475 | ||
| NGC 4945 (n) | H2O+ | +640(7) | 89(7) | –278(26) | 475 | ||
| NGC 4945 (n) | OH+ | +654(5) | 70(5) | –220(10) | 350 | ||
| NGC 4945 (b) | H2O | +573(1) | 121(1) | –203(1) | 475 | ||
| NGC 4945 (b) | H2O+ | +557(7) | 123(7) | –196(14) | 475 | ||
| NGC 4945 (b) | OH+ | +574(5) | 120(5) | –270(5) | 350 | ||
| NGC 253 (e) | H2O | +252(1) | 146(2) | +154(3) | 360 | ||
| NGC 253 (e) | H2O+ | +308(6) | 158(6) | +83(5) | 360 | ||
| NGC 253 (e) | OH+ | +301(24) | 176(18) | +130(4) | 230 | ||
| NGC 253 (a) | H2O | +217(1) | 122(1) | –248(2) | 360 | ||
| NGC 253 (a) | H2O+ | +196(6) | 132(6) | –234(12) | 360 | ||
| NGC 253 (a) | OH+ | +216(6) | 158(5) | –290(9) | 230 | ||
| Arp 220 | H2O | +5445(5) | 235(11) | –26(2) | 48 | ||
| Arp 220 | H2O+ | +5443(9) | 312(21) | –25(2) | 48 | ||
| Arp 220 | OH+ | +5418(4) | 283(9) | –25(1) | 33 | ||
| M 82c | H2O | +239(3) | 73(8) | –11(4) | 151 | ||
| M 82c | H2O+ | +239(2) | 75(4) | –20(2) | 151 | ||
| M 82SW | H2O | +209(3) | 41(7) | –18(4) | 120 | ||
| M 82SW | H2O+ | +217(3) | 57(5) | –24(3) | 120 | ||
| M 82NE | H2O | +288(3) | 104(6) | –30(2) | 140 | ||
| M 82NE | H2O+ | +280(2) | 113(5) | –40(2) | 140 | ||
| Cen A (e) | H2O | +497(6) | 49(11) | +9(3) | 34 | ||
| Cen A (e) | H2O+ | +477(6) | 48(14) | +8(3) | 34 | ||
| Cen A (a) | H2O | +542(9) | 70(20) | –8(2) | 34 | ||
| Cen A (a) | H2O+ | +580(15) | 58(19) | –4(1) | 34 | ||
Notes. Numbers in parentheses are formal errors from the Gaussian fits in units of the last decimal; (n) = narrow component, (b) = broad component, (e) = emission component, (a) = absorption component. The line temperatures in Col. 5 are in TA units and are relative to the SSB continuum values reported in Col. 6 which have a 10−15% calibration uncertainty.
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