Star-forming regions of the Aquila rift cloud complex - I. NH3 tracers of dense molecular cores

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Table B.1

Observed parameters of the NH₃(1, 1) and (2, 2) lines and calculated model parameters for Kawamura 01 and 05, Dobashi 279 P7 and P8, and Dobashi 321 P2.

Peak	Δα	Δδ	V_LSR	Δv	T_MB	T_ex	T_rot	T_kin	n_H₂/10⁴	τ₁₁	τ₂₂	N_tot/10¹⁵
Id.	(′′)	(′′)	(km s^-1)	(km s^-1)	(K)	(K)	(K)	(K)	(cm^-3)			(cm^-2)

Ka01
	0, 0		9.60	0.32	1.5	4.3	8.7	9.1	1.2	10.9	0.2	1.2
α	0,−40		9.55	0.32	2.5	5.5	9.2	9.6	2.5	10.5	0.3	1.3
	+40,−40		9.60	0.30	1.4	4.8	<8.5	...	...	4.1	<0.1	≥0.5
	+40,−80		9.54	0.30	0.8	4.1	<9.6	...	...	3.2	<0.1	≥0.3
	−40,0		9.62	0.23	1.7	4.7	<8.9	...	...	8.2	<0.2	≥1.0
	−40,−40		9.60	0.27	1.3	4.3	<9.7	...	...	6.6	<0.2	≥0.5
Ka05
α	0,0		8.40	0.37	2.5	5.6	10.2	10.7	2.3	5.6	0.3	0.8
	0,−40		8.40	0.33	2.1	5.1	10.8	11.5	1.6	8.0	0.4	0.7
Do279P7
α	−80,40		6.04	0.75	1.5	6.4	12.6	13.7	1.1	4.3	0.4	0.6
	−40,40		6.14	0.72	1.4	4.5	13.3	14.7	1.0	3.8	0.4	0.5
	−80,0		6.59	0.55	1.4	5.1	13.5	14.9	1.4	2.4	0.3	0.3
	−80,80		5.91	0.73	0.5	3.3	11.5	12.4	0.3	4.4	0.3	0.5
Do279P8
α	0,0		8.52	0.27	2.5	5.7	<8.0	...	...	8.0	<0.1	≥1.1
	0,−40		8.57	0.30	2.4	5.7	<7.7	...	...	6.9	<0.1	≥1.2
Do321P2
α	−80,120		6.88	0.48	3.0	6.8	11.9	12.9	3.3	4.0	0.3	0.6
β	−80,40		7.05	0.43	2.7	6.7	11.4	12.2	3.4	3.5	0.2	0.5
γ	−120,−40		6.93	0.38	1.7	5.5	<9.1	...	...	3.0	<0.1	≥0.5
δ	− 80,240		7.12	0.48	1.6	4.7	<9.7	...	...	4.8	<0.1	≥0.7
ε	80,−40		6.66	0.73	1.3	<5.7	...	...	...	...	...	...

Notes.Δv is the linewidth (FWHM); τ₁₁, τ₂₂ are defined in Eqs. (A.2) and (A.3), and N_tot — in Eq. (A.19).

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