The ISO Long Wavelength Spectrometer line spectrum of VY Canis Majoris and other oxygen-rich evolved stars

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Table 3:

Possible rotational lines from the vibrationally excited $\nu _{2} = 1$ state of water in the LWS spectrum of VY CMa.
Transition	Wavelength	Energy of	Flux^a
	( $\mu$ m)	upper state (K)	(10^-19 W cm^-2)
3₀₃-2₁₂	182.36	2491.8	$1.3\pm0.3$
6₃₃-6₂₄	140.06	3284.2	$1.2\pm0.2$
4₂₃-4₁₄	115.71	2745.2	$2.3\pm0.8$

Notes. ^(a) Errors do not include systematic uncertainty in the baseline subtraction ( $\sim$ 30%).

Source LaTeX | All tables | In the text

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