ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA

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Table 2

Extract of Table A.5 which lists all measured lines in each source.

Source	Line	v₀ (GHz)	Res.⁽¹⁾	Ap.⁽²⁾ (″)	F_peak (Jy)	I (Jy kms⁻¹)	RW⁽³⁾ (kms⁻¹)	BW⁽⁴⁾ (kms⁻¹)	W_vel (kms⁻¹)	r⁽⁵⁾ (″)
AH Sco	SiO v = 2 J = 5−4	214.089	high	0.04	1.103	7.765	23.5	−21.6	45.1	0.08
AH Sco	SiO v = 2 J = 5−4	214.089	high	0.12	1.679	11.892	23.5	−18.9	42.4	0.08
AH Sco	SiO v = 2 J = 5−4	214.089	high	0.08	1.644	11.594	23.5	−18.9	42.4	0.08
AH Sco	SiO v = 2 J = 5−4	214.089	med	3.6	2.604	15.148	15.3	−14.7	30.1	0.37
AH Sco	SiO v = 2 J = 5−4	214.089	med	1.2	2.616	15.449	18.1	−14.7	32.8	0.37
AH Sco	SiO v = 2 J = 5−4	214.089	med	0.4	2.552	14.964	20.8	−20.2	41.0	0.37

Notes. ⁽¹⁾Spatial resolution of the data.⁽²⁾Aperture diameter used to extract the spectrum. ⁽³⁾Velocity of the red line wing. ⁽⁴⁾Velocity of the blue line wing.⁽⁵⁾ Angular emission radius. The full version of the table (which also includes columns for uncertainties) is available at the CDS.

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