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Table 2

Fitparameters for the targeted HDO and HO transitions.

Species νrest (GHz) (mJy beam−1) FWHM (km s−1) vlsr (km s−1) N (cm−2)
L483

HDO 225.896720(a) 37 ± 4 4.8 ± 0.3 1.7 ± 0.1 (1.7 ± 0.2) × 1015
HDO 225.896720(b) 78 ± 8 5.6 ± 0.2 7.4 ± 0.1 (4.3 ± 0.4) × 1015
HDO 241.561550(a) 42 ± 5 5.1 ± 0.2 2.1 ± 0.2 (1.8 ± 0.2) × 1015
HDO 241.561550(b) 82 ± 8 5.5 ± 0.4 7.7 ± 0.2 (3.8 ± 0.4) × 1015
HO 203.407520(a) 10.2 ± 1.5 5.2 ± 1.0 2.4 ± 0.4 (2.3 ± 0.6) × 1015
HO 203.407520(b) 10.5 ± 1.5 5.2 ± 1.0 9.2 ± 0.4 (2.4 ± 0.6) × 1015

B335

HDO 225.896720 190 ± 19 4.74 ± 0.04 7.97 ± 0.16 (3.1 ± 0.3) × 1015
HDO 241.561550 187 ± 19 4.71 ± 0.05 7.89 ± 0.15 (2.6 ± 0.3) × 1015
HO 203.407520 32 ± 4 5.78 ± 0.36 7.49 ± 0.14 (2.9 ± 0.4) × 1015

BHR71–IRS1

HDO 225.896720 65 ± 7 4.51 ± 0.16 − 4.97 ± 0.05 (1.9 ± 0.2) × 1015
HDO 241.561550 66 ± 7 4.57 ± 0.15 − 4.67 ± 0.05 (2.2 ± 0.2) × 1015
HO 203.407520 17 ± 3 3.80 ± 0.48 − 4.07 ± 0.20 (2.0 ± 0.4) × 1015

Notes. Fν includes 10% calibration uncertainty. FWHM uncertainty is determined as the maximum between the uncertainty in the fitted Gaussian and the channel width. Column densities N were calculated assuming optically thin emission from a gas in LTE at 124 K. Furthermore, the column densities assume that the emission fills the beam. Toward L483, (a) denotes the weaker blueshifted component and (b)the brighter redshifted component.

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