Challenging shock models with SOFIA OH observations in the high-mass star-forming region Cepheus A

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Volume 585 (January 2016)

A&A, 585 (2016) A45

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Table 5

Observed integrated intensities (, in K km s^-1) of the emission lines.

	Blueshifted			Redshifted
Component	HV	LV	total	LV	HV	total
Velocity interval (km s^-1)	[–90; –19]	[–19; –11]	[–90; –11]	[–11; –3]	[–3; 30]	[–11; 30]
Corresponding Δν (km s^-1)	71	8	79	8	33	41

OH 1835 GHz	20.7	15.5	36.2	18.1	15.5	33.6
OH 1838 GHz	20.4	16.7	37.1	16.3	18.8	35.1
OH 2514 GHz	21.5^a	–	–	–	–	–

CO (16–15)	16.4	27.1	43.5	28.0	13.9	41.9

Notes.The uncertainty in the integrated intensities mostly comes from the line temperature calibration of the order of ±10%. LV and HV stand for low-velocity and high-velocity. The “total” value was used in scenario 1 (Sect. 5.1), while the LV and HV values were used in scenario 2 (Sect. 5.2).

^(a)

Integrated between –90 and –20 km s^-1.

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