Physical structure and water line spectrum predictions of the intermediate mass protostar OMC2-FIR4

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Volume 506 / No 3 (November II 2009)

A&A, 506 3 (2009) 1229-1241

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Table 5:

Predictions of the line fluxes (after subtraction of the continuum) of the water lines observable with the Herschel spectrometers, HIFI and PACS.
PACS range
Transition	Wavelength	Flux
	( $\mu$ m)	(erg s^-1 cm^-2)
H₂¹⁶O
2 $_{ 2 1} \rightarrow$ 3_{3 0}	66.44	2.99E-14
2 $_{ 2 0} \rightarrow$ 3_{3 1}	67.09	1.13E-14
3 $_{ 0 3} \rightarrow$ 3_{3 0}	67.27	2.28E-14
2 $_{ 1 2} \rightarrow$ 3_{2 1}	75.38	1.55E-13
3 $_{ 1 2} \rightarrow$ 4_{2 3}	78.74	4.51E-14
2 $_{ 1 1} \rightarrow$ 3_{2 2}	89.99	5.09E-14
4 $_{ 0 4} \rightarrow$ 5_{1 5}	95.63	1.05E-14
4 $_{ 1 4} \rightarrow$ 5_{0 5}	99.49	4.21E-14
1 $_{ 1 1} \rightarrow$ 2_{2 0}	100.98	7.80E-14
1 $_{ 1 0} \rightarrow$ 2_{2 1}	108.07	1.43E-13
3 $_{ 0 3} \rightarrow$ 4_{1 4}	113.54	8.45E-14
4 $_{ 2 3} \rightarrow$ 4_{3 2}	121.72	1.14E-14
3 $_{ 1 3} \rightarrow$ 4_{0 4}	125.36	5.34E-14
4 $_{ 1 4} \rightarrow$ 4_{2 3}	132.41	2.92E-14
3 $_{ 2 1} \rightarrow$ 3_{3 0}	136.49	1.35E-14
2 $_{ 0 2} \rightarrow$ 3_{1 3}	138.53	7.84E-14
3 $_{ 1 3} \rightarrow$ 3_{2 2}	156.20	2.25E-14
2 $_{ 1 2} \rightarrow$ 3_{0 3}	174.62	7.42E-14
1 $_{ 0 1} \rightarrow$ 2_{1 2}	179.53	1.17E-13
2 $_{ 1 2} \rightarrow$ 2_{2 1}	180.49	4.97E-14
HIFI range
Transition	Frequency	Flux
	(GHz)	(K km s^-1)
H₂¹⁶O
1 $_{ 0 1} \rightarrow$ 1_{1 0}	556.96	14.8
2 $_{ 0 2} \rightarrow$ 2_{1 1}	752.04	1.06E+00
1 $_{ 1 1} \rightarrow$ 2_{0 2}	987.95	1.31E+00
3 $_{ 0 3} \rightarrow$ 3_{1 2}	1097.34	1.46E+00
0 $_{ 0 0} \rightarrow$ 1_{1 1}	1113.35	4.32E+00
2 $_{ 2 1} \rightarrow$ 3_{1 2}	1153.09	2.50E+00
3 $_{ 1 2} \rightarrow$ 3_{2 1}	1162.93	6.97E-01
2 $_{ 1 1} \rightarrow$ 2_{2 0}	1228.81	5.33E-01
4 $_{ 1 3} \rightarrow$ 4_{2 2}	1207.62	2.45E-01
5 $_{ 1 4} \rightarrow$ 5_{2 3}	1410.65	1.47E-01
2 $_{ 1 2} \rightarrow$ 2_{2 1}	1660.99	2.33E+00
4 $_{ 0 4} \rightarrow$ 4_{1 3}	1602.23	1.46E-01
1 $_{ 0 1} \rightarrow$ 2_{1 2}	1669.87	5.46E+00
2 $_{ 1 2} \rightarrow$ 3_{0 3}	1716.83	3.37E+00
5 $_{ 2 3} \rightarrow$ 5_{3 2}	1867.75	3.13E-02
H₂¹⁸O
1 $_{ 0 1} \rightarrow$ 1_{1 0}	556.96	1.88E-01

0 $_{ 0 0} \rightarrow$ 1_{1 1}	1113.35	1.48E-01

The predictions refer to the reference model (model 1 of Table 4).

Source LaTeX | All tables | In the text

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