The effects of stellar feedback on molecular clumps in the Lagoon Nebula (M8)

Open Access

Table E.1

Line parameters of identified RRLs in the M8 region.

Clump	Transition	I	v_LSR	∆v
		K km s⁻¹	km s⁻¹	km s⁻¹
HG	II 39−44α	12.69 ± 0.04	3.5 ± 0.1	26.7 ± 0.1
	He39−	0.84 ± 0.03	1.9 ± 0.3	19.7 ± 0.8
	44α
	C 39−44α	0.11 ± 0.02	11.1 ± 0.2	4.1 ± 0.6
	H 48−56β	3.78 ± 0.09	3.3 ± 0.3	26.8 ± 0.8
	H 54−63γ	1.75 ± 0.03	3.7 ± 0.3	26.6 ± 0.7
WC1	H 39−44α	1.46 ± 0.04	−2.4 ± 0.3	22.0 ± 0.7
WC2	H 39−44α	0.92 ± 0.05	0.5 ± 0.7	25.8 ± 1.7
WC3	H 39−44α	1.04 ± 0.06	0.2 ± 0.6	22.8 ± 1.4
WC4	H 39−44α	1.97 ± 0.06	6.4 ± 0.5	29.2 ± 1.0
WC5	H 39−44α	1.64 ± 0.05	1.7 ± 0.4	23.8 ± 0.8
WC6	H 39−44α	1.12 ± 0.05	1.3 ± 0.5	23.9 ± 1.4
EC1	H 39−44α	0.39 ± 0.04	−0.1 ± 0.8	18.3 ± 2.1
EC2	H 39-44α	0.39 ± 0.05	0.1 ± 1.0	16.0 ± 2.4
SC6	H 39−44α	0.79 ± 0.05	−0.4 ± 0.8	21.9 ± 1.4

Notes. Fits for the α RRLs with N=39-44 include lines with N=39-42 and N=44. Similarly, our observations do not cover RRLs with N=53 and 54 for β and N=61 for γ transitions, due to which these are not used for the combined spectra.

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