NIR jets from a clustered region of massive star formation - Morphology and composition in the IRAS 18264-1152 region

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Volume 659 (March 2022)

A&A, 659 (2022) A23

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Table B.1

Integrated line fluxes of H₂ lines detected in each jet knot.

Transition	Wavelength	Integrated line fluxes (10⁻¹⁵ erg s⁻¹ cm⁻²)
	in vacuum	KMOS							SINFONI
	(μm)	K1	K2	K3	K4	K5	K6	K7	K2*	K3	K8
1-0 S(3)	1.9576	3.93±0.42	4.42±0.46	3.71±0.42	2.71±0.31	12.4±1.28	-	12.1±1.27	15.5±1.70	24.1±2.52	8.72±1.22
1-0 S(2)	2.0338	1.50±0.16	3.20±0.34	2.65±0.30	1.13±0.14	5.02±0.52	1.75±0.21	4.14±0.43	5.14±0.60	6.74±0.74	3.03±0.43
2-1 S(3)	2.0735	0.73±0.09	1.30±0.15	0.77±0.12	0.41±0.06	1.96±0.21	0.64±0.11	1.54±0.17	1.57±0.27	2.29±0.28	1.42±0.26
1-0 S(1)	2.1218	3.99±0.43	8.40±0.90	7.74±0.83	3.11±0.33	14.8±1.52	5.55±0.60	12.4±1.28	13.2±1.41	19.1±1.96	9.17±1.02
2-1 S(2)	2.1542	0.32±0.04	0.81±0.13	-	0.35±0.05	0.98±0.12	0.38±0.08	0.72±0.09	0.75±0.21	1.14±0.20	0.44±0.10
1-0 S(0)	2.2233	1.00±0.11	2.15±0.23	2.16±0.25	0.83±0.10	3.83±0.39	1.55±0.20	2.97±0.31	2.53±0.36	5.14±0.57	2.10±0.35
2-1 S(1)	2.2477	0.51±0.06	0.95±0.11	0.83±0.12	0.46±0.07	1.76±0.19	0.71±0.11	1.17±0.13	1.05±0.22	2.43±0.30	-
2-1 S(0)	2.3556	0.19±0.04	0.65±0.11	-	-	0.68±0.09	-	0.42±0.06	-	0.65±0.13	-
1-0 Q(1)	2.4066	4.30±0.48	6.66±0.71	6.48±0.72	4.49±0.51	15.7±1.65	2.29±0.46	13.3±1.41	14.8±1.67	23.1±2.44	11.5±1.49
1-0 Q(2)	2.4134	1.53±0.23	2.65±0.31	2.85±0.36	1.83±0.25	5.36±0.61	-	4.68±0.57	3.83±0.61	6.91±0.82	3.20±0.55
1-0 Q(3)	2.4237	3.52±0.39	5.77±0.62	5.97±0.67	3.37±0.38	13.0±1.36	1.48±0.18	10.3±1.08	13.1±1.53	19.7±2.11	10.9±1.51
1-0 Q(4)	2.4375	0.95±0.17	1.91±0.24	1.78±0.26	1.29±0.20	5.46±0.66	-	3.81±0.53	3.22±0.50	5.86±0.71	3.67±0.66

Notes. The dashes (’-’) stand for non detections or the Gaussian fit returned S∕N < 10.

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