Linking low- to high-mass young stellar objects with Herschel-HIFI observations of water

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Volume 585 (January 2016)

A&A, 585 (2016) A103

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Table A.5

Gaussian decomposition results for the intermediate-mass objects.

Source	Comp.^a	FWHM	ν_peak	ν_LSR	H₂O 2₀₂–1₁₁		H₂O 2₁₁–2₀₂		H₂O 3₁₂–3₀₃
						^b		^b		^b
		(km s^-1)	(km s^-1)	(km s^-1)	(K)	(K km s^-1)	(K)	(K km s^-1)	(K)	(K km s^-1)

NGC 7129 FIRS2	C	29.3 ± 0.3	–13.99 ± 0.17	–9.8	0.192 ± 0.004	5.99 ± 0.14	0.160 ± 0.004	4.99 ± 0.13	0.166 ± 0.003	5.18 ± 0.11
	E	8.46 ± 0.11	–7.20 ± 0.04	–9.8	0.368 ± 0.005	3.31 ± 0.06	0.282 ± 0.006	2.54 ± 0.06	0.285 ± 0.004	2.57 ± 0.05
L1641 S3MMS1	C	34 ± 3	6.4 ± 0.9	5.3	0.073 ± 0.013	2.6 ± 0.5	0.084	3.04	−	−
	E	15.3 ± 0.5	8.57 ± 0.16	5.3	0.197 ± 0.014	3.2 ± 0.3	0.155 ± 0.005	2.53 ± 0.11	−	−
NGC 2071	C	29.60 ± 0.12	9.14 ± 0.05	9.6	1.722 ± 0.008	54.3 ± 0.3	1.42 ± 0.007	44.7 ± 0.3	1.311 ± 0.006	41.3 ± 0.3
	E	6.122 ± 0.04	10.17 ± 0.02	9.6	2.039 ± 0.017	13.3 ± 0.2	1.924 ± 0.012	12.5 ± 0.1	1.283 ± 0.009	8.36 ± 0.08
	S	31.2 ± 0.7	46.9 ± 0.3	9.6	0.277 ± 0.005	9.2 ± 0.3	0.199 ± 0.004	6.6 ± 0.2	0.229 ± 0.003	7.6 ± 0.2
	A	3.65 ± 0.09	6.54 ± 0.04	9.6	–0.814 ± 0.018	–3.16 ± 0.11	−	−	−	−
Vela IRS17	C	23.8 ± 0.4	7.53 ± 0.14	3.9	0.277 ± 0.005	7.01 ± 0.16	0.158 ± 0.005	4.00 ± 0.14	−	−
	E	4.19 ± 0.07	4.47 ± 0.03	3.9	0.462 ± 0.009	2.06 ± 0.05	0.608 ± 0.011	2.71 ± 0.07	−	−
Vela IRS19	C	33.3 ± 0.8	16.7 ± 0.3	12.2	0.141 ± 0.003	5.00 ± 0.16	0.068 ± 0.004	2.41 ± 0.15	−	−
	E	4.14 ± 0.18	11.92 ± 0.07	12.2	0.183 ± 0.008	0.81 ± 0.05	0.215 ± 0.012	0.95 ± 0.07	−	−
AFGL490	C	31.9 ± 1.0	–11.7 ± 0.4	–13.5	0.107 ± 0.004	3.63 ± 0.18	0.033 ± 0.004	1.12 ± 0.14	−	−
	E	4.56 ± 0.11	–13.40 ± 0.04	–13.5	0.299 ± 0.007	1.45 ± 0.05	0.364 ± 0.011	1.77 ± 0.07	−	−
OMC-2-FIR 4	C	18.62 ± 0.07	11.33 ± 0.03	11.3	2.085 ± 0.018	41.3 ± 0.4	1.210 ± 0.009	24.0 ± 0.2	1.031 ± 0.010	20.4 ± 0.2
	E	6.26 ± 0.08	13.40 ± 0.02	11.3	1.03 ± 0.03	6.87 ± 0.19	0.677 ± 0.009	4.51 ± 0.08	0.566 ± 0.014	3.77 ± 0.11

Notes.

^(a)

The types of components are: C = cavity shock; E = envelope emission; S = spot shock; A = envelope absorption.

^(b)

Integrated intensity of each velocity component approximated to the Gaussian fit.

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