Circumstellar molecular composition of the oxygen-rich AGB star IK Tauri - II. In-depth non-LTE chemical abundance analysis

L. Decin; E. De Beck; S. Brünken; H. S. P. Müller; K. M. Menten; H. Kim; K. Willacy; A. de Koter; F. Wyrowski

doi:10.1051/0004-6361/201014136

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Volume 516 (June-July 2010)

A&A, 516 (2010) A69

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Table 8:

Line frequencies, upper energy levels and Einstein A-coefficients for the ortho-H₂O lines, which will be observed with Herschel/HIFI.
Vibrational	Transition	Frequency	$E_{\rm upper}$	A
state		[GHz]	[cm^-1]	[s^-1]
v=0	1_1,0-1_0,1	556.933	42.371	$3.497 \times 10^{-3}$
v=0	5_3,2-4_4,1	620.882	50.880	$1.106 \times10^{-4}$
v=0	3_1,2-3_0,3	1097.488	173.365	$1.664 \times10^{-2}$
v=0	3_1,2-2_2,1	1153.219	173.365	$2.693 \times10^{-3}$
v=0	6_3,4-5_4,1	1158.391	648.967	$1.417 \times10^{-3}$
v=0	3_2,1-3_1,2	1162.849	212.154	$2.307 \times10^{-2}$
v=0	8_5,4-9_2,7	1595.961	1255.144	$2.947 \times10^{-4}$
v=0	3_0,3-2_1,2	1716.731	136.757	$5.109 \times10^{-2}$
v=0	7_3,4-7_2,5	1797.168	842.355	$9.143\times10^{-2}$
v=0	5_3,2-5_2,3	1867.562	508.806	$8.198 \times10^{-2}$
v=1	1_1,0-1_0,1	658.081	1618.683	$5.575 \times10^{-3}$
v=1	8_2,7-7_3,4	967.403	2495.278	$5.800 \times10^{-4}$
v=1	2_1,2-1_0,1	1753.922	1677.187	$6.335 \times10^{-2}$

Source LaTeX | All tables | In the text

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