CO outflows from young stars in the NGC2023 cluster

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Table 1

Observing setup.

Receiver	Molecular transition	Frequency (GHz)	^θFWHM	η_mb	rms (K)
FLASH+	¹³CO(3−2)	330.587965	18.5	0.68	0.3
FLASH+	CO(3−2)	345.795990	17.7	0.68	0.2
FLASH+	CO(4−3)	461.040768	13.3	0.58	0.4
CHAMP+	CO(6−5)	691.473076	9.1	0.49	1.3
CHAMP+	CO(7−6)	806.651806	7.7	0.48	2.5
GREAT L1	CO(11−10)	1267.014486	23.0	0.67	1.1
upGREAT HFA	[O I] 63 µm	4744.777490	6.3	0.63	1.6

Notes. The quoted rms sensitivities are in T_mb for a velocity resolution of 0.5 km s⁻¹. θ_FWHM is the half-power beam width, and η_mb is the main-beam coupling efficiency.

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