Discovery of water vapour in the carbon star V Cygni from observations with Herschel/HIFI

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Volume 521 (October 2010)

A&A, 521 (2010) L5

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Herschel/HIFI: first science highlights

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Table 3:

Predicted line strengths for V Cygni.
Transition	Frequency	Wavelength	Line strength
	(GHz)	( $\mu$ m)	$\int T_{\rm MB}~ {\rm d}v$ in K $\rm km~s^{-1}$ ^a
			Model A	Model B
1₁₁-0₀₀	1113.343	269.272	2.53^a	2.53^b
2₀₂-1₁₁	987.927	303.456	2.46	2.79
2₁₁-2₀₂	752.033	398.643	1.18	1.17
2₂₀-2₁₁	1228.789	243.974	0.56	0.56
4₂₂-3₃₁	916.171	327.223	0.47	0.02
1₁₀-1₀₁	556.936	538.289	1.16	1.06
2₁₂-1₀₁	1669.905	179.527	6.40	5.90
2₂₁-2₁₂	1661.008	180.488	1.92	1.79
3₀₃-2₁₂	1716.770	174.626	5.43	4.93
3₁₂-2₂₁	1153.126	259.982	1.37	0.85
3₁₂-3₀₃	1097.365	273.193	1.67	1.49
3₂₁-3₁₂	1162.911	257.795	0.65	0.59
4₃₂-5₀₅	1713.882	174.920	0.64	0.03
Transition	Frequency	Wavelength	Line strength
	(GHz)	( $\mu$ m)	( $10^{-16}~\rm W~m^{-2}$ )
			Model A	Model B
2₁₁-2₀₂	2968.748	100.983	1.27	0.82
3₃₁-2₂₀	4468.572	67.089	1.16	0.42
2₂₁-1₁₀	2773.976	108.073	2.20	1.67
3₂₁-2₁₂	3977.045	75.381	2.61	1.11
4₁₄-3₀₃	2640.473	113.537	1.70	0.70
3₃₀-2₂₁	4512.385	66.438	2.51	1.12
4₃₂-3₁₂	3807.256	78.742	1.72	0.23
5₀₅-4₁₄	3013.199	99.493	1.23	0.22
4₃₂-3₂₁	5107.284	58.699	1.73	0.35
6₁₆-5₀₅	3654.602	82.031	1.20	0.02

Notes. ^(a) Integrated main beam temperature; ^(b) observed line strength.

Source LaTeX | All tables | In the text

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