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

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Table 5:

Fitted fluxes for the CO lines observed above 120 $\mu$ m for VY CMa.
Transition	Wavelength	Auto	Manual
	( $\mu$ m)	fit flux	fit flux^a
		(10^-19 W cm^-2)	(10^-19 W cm^-2)
J = 14-13	185.999	1.72	$1.96 \pm 0.4$
J = 15-14	173.631	1.35	$1.88 \pm 1.3$
J = 16-15	162.812	2.37	$2.69 \pm 1.4$
J = 17-16	153.267	1.54	$2.00 \pm 0.6$
J = 18-17	144.784	-Blend-	-Blend-
J = 19-18	137.196	1.06	$1.31 \pm 1.1$
J = 20-19	130.369	-Blend-	-Blend-
J = 21-20	124.193	1.60	$0.92 \pm 2.0$

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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