The distribution of water in the high-mass star-forming region NGC 6334 I

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Table 3:

Parameters of the narrow absorption features seen in the two ground-state H₂¹⁶O transitions.
Line	$v\rm _{\rm lsr}$	$T\rm _{\rm MB}$	$\int T_{\rm MB} {\rm d}v$	Cont. level
	km s^-1	K	Kkm s^-1	K
	- $6.2\pm 0.3$	$0.21\pm0.17$	$6.2\pm0.31$	$7.7\pm0.4$
1₁₁-0₀₀	$-0.34\pm 0.1$	$1.87\pm0.17$	$7.8\pm0.39$	$7.7\pm0.4$
	$+6.1\pm 0.10$	$0.33\pm0.17$	$7.8\pm0.39$	$9.0\pm0.45$
	$-6.8\pm 1.0$	0.22 $\pm0.024$	$2.04\pm0.10$	$1.54\pm0.08$
1₁₀-1₀₁	$-0.25\pm 0.1$	$0.81\pm0.024$	$2.69\pm0.13$	$1.53\pm0.08$
	+6.3 $\pm 0.10$	0.19 $\pm0.024$	$2.36\pm0.76$	$1.51\pm0.08$

Notes. $\int T_{\rm MB} {\rm d}v$ is the intensity integrated over the velocity ranges of the individual components (Table 1). The continuum level given is an average value for the individual components.

Source LaTeX | All tables | In the text

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