The molecular environment of the Galactic star forming region G19.61–0.23

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Table 1:

Summary of the parameters of the spectral line observations.
Line	$\nu$	$\Theta_{\rm beam}$	$T_{\rm sys}$	$\Delta~v$	$\eta_{\rm mb}$
	(GHz)	(arcsec)	(K)	(km s^-1)
(1)	(2)	(3)	(4)	(5)	(6)
FCRAO 14 m
¹³CO(1-0)	110.201	46	294-680	0.2	0.49
C¹⁸O(1-0)	109.782	46	291-697	0.2	0.49
C¹⁷O(1-0)	112.359	46	290-371	0.2	0.47
IRAM 30 m
¹³CO(2-1)	220.399	11	639-1129	0.1	0.52
C¹⁸O(2-1)	219.569	11	659-1061	0.1	0.52
C¹⁷O(2-1)	224.714	11	383-517	0.1	0.536

Notes. Column (1): the observed line; Col. (2): the frequency of the transition; Col. (3): the beam size of the observations; Col. (4): the typical system temperature, $T_{\rm sys}$ , of the observations; Col. (5): the velocity resolution, $\Delta~v$ , of the observations; Col. (6): the beam efficiency used for every specific frequency.

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