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Table D.1
OH rotational excitation and number of emitting molecules 
based on emission lines for low- and intermediate-mass sources.
| Source | Trot(K) |
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| Low-mass YSOs | ||||
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| NGC 1333 I4A | 270(700) | 52.4(0.9) | ||
| L1527 | 80(40) | 51.5(0.6) | ||
| Ced110 I4 | 380(1400) | 51.4(0.9) | ||
| IRAS15398 | 85(90) | 51.5(1.0) | ||
| L483 | 200(380) | 52.0(0.9) | ||
| L1489 | 140(150) | 51.6(0.7) | ||
| TMR1 | 490(2150) | 52.0(0.8) | ||
| TMC1 | 170(290) | 51.7(0.9) | ||
| HH46 | 160(350) | 52.6(1.1) | ||
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| Intermediate-mass YSOs | ||||
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| NGC 2071 | 37(10) | 55.7(0.8) | ||
| Vela IRS17 | 35(10) | 55.1(0.7) | ||
| Vela IRS19 | 36(15) | 55.1(1.1) | ||
| NGC 7129 FIRS2 | 170(270) | 53.9(0.9) | ||
| L1641 S3MMS1 | 36(10) | 54.7(0.8) | ||
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