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

Open Access

Table G.1

Column density values and upper limits for 50 species at HG (extract).

Clump	Species	N₁ (Species)	N₂(Species)
		(cm ⁻²)	(cm ⁻²)
IIG	¹³CN	< 2.6 × 10¹³	−
HG	c-C₃H	< 1.7 × 10¹³	−
HG	C¹³CH	< 8.2 × 10¹³	−
HG	C₂D	< 1.4 × 10¹⁴	−
HG	C₂H	1.8 × 10¹⁵
HG	CN	1.0 × 10¹⁵	1.2 × 10¹⁴
HG	HCO	1.1 × 10¹⁴
HG	NO	< 1.1 × 10¹⁵	−
HG	NS	< 3.7 × 10¹³	−
HG	¹³CH₃OH−A⁺	< 5.8 × 10¹³	−
HG	¹³CO	1.8 × 10¹⁷	1.3 × 10¹⁶
HG	¹³C¹⁸O	< 2.0 × 10¹⁵	−
HG	¹³CS	1.1 × 10¹³
HG	¹³ C³⁴ S	< 1.7 × 10¹²	−
IIG	C₃II⁺	< 1.1 × 10¹²	−
HG		2.6 × 10¹³
IIG	C₂S	7.1 × 10¹²
HG	CF⁺	8.1 × 10¹²
HG	CH₃C₂H	3.8 × 10¹³
HG	CH₃CHO−A	< 2.4 × 10¹³	−
HG	CH₃CN	1.1 × 10¹²
HG	CH₃OH−A⁺	1.9 × 10¹⁴
HG	CH₃SH−E	< 4.5 × 10¹³	−
HG	CO	4.5 × 10¹⁷	1.3 × 10¹⁷
HG	C¹⁷O	5.6 × 10¹⁶
HG	C¹⁸O	2.9 × 10¹⁶	5.1 × 10¹⁴
HG	CS	2.4 × 10¹⁴	4.7 × 10¹²
HG	C³³S	9.3 × 10¹²
HG	³⁴CS	3.3 × 10¹³
HG	DC₃N	< 8.8 × 10¹¹	−
HG	DCN	6.5 × 10¹²
HG	DCO⁺	6.1 × 10¹¹
HG	DNC	< 2.9 × 10¹²	−
HG	$H_{2}^{13} CO$ ${\rm{H}}_2^{13}{\rm{CO}}$	< 2.6 × 10¹²	−
HG	H₂C₂O	< 1.2 × 10¹³	−
HG	H₂CO	5.4 × 10¹³	1.4 × 10¹³
HG	H₂CS	2.6 × 10¹³
HG	H₂C³⁴S	< 1.1 × 10¹³	−
HG	H₂S	< 1.1 × 10¹⁴	−
HG	H¹³CC₂H	< 1.1 × 10¹²	−
HG	H¹³CN	1.2 × 10¹³
HG	H¹³CO⁺	3.7 × 10¹²	2.9 × 10¹¹
HG	HC₃N	1.6 × 10¹³
HG	HC₅N	< 2.6 × 10¹²	−
IIG	HC¹³CCN	< 9.9 × 10¹¹	−
HG	${HC}_{2}^{13} CN$ ${{\rm{HC}}_2^{13}{\rm{CN}}}$	< 9.9 × 10¹¹	−
HG	${HC}_{3}^{15} N$ ${{\rm{HC}}_3^{15}{\rm{N}}}$	< 8.2 × 10¹¹	−
HG	HCN	2.8 × 10¹⁴
HG	HC¹⁵N	2.3 × 10¹²
HG	HCNO	< 7.4 × 10¹¹	−

Notes. Uncertainties are estimated to be of order 10% based on the calibration uncertainty of the telescopes. If two velocity components are detected, the column densities N₁ and N₂ are calculated separately. For undetected species, an upper limit of the respective column density is calculated based on the baseline RMS. Corresponding values are marked with a <. The complete table containing all detected species at all M8 clumps is available at the CDS.

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