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

Open Access

Table A.1

Coordinates of all the clumps observed with the APEX and the IRAM 30m telescopes.

Clump	RA (J2000)	Dec. (J2000)
HG	18^h 03^m40.7^s	−24°22′40″
WC1	18^h03^m36.6^s	−24°22′14″
WC2	18^h03^m33.7^s	−24° 21′49″
WC3*	18^h03^m44.8^s	−24° 21′23″
WC4	18^h03^m44.6^s	−24°22′16″
WC5	18^h03^m35.9^s	−24°23′10″
WC6	18^h03^m34.6^s	−24°23′25″
WC7	18^h03^m26.2^s	−24°22′34″
WC8	18^h03^m28.5^s	−24° 21′50″
WC9	18^h03^m25.3^s	−24° 21′39″
SW1	18^h03^m25.8^s	−24°28′ 11″
EC1	18^h04^m21.6^s	−24°24′27″
EC2	18^h04^m22.5^s	−24°23′25″
EC3	18^h04^m22.4^s	−24°22′57″
EC4	18^h04^m19.2^s	−24°22′26″
EC5	18^h04^m18.0^s	−24°22′05″
E	18^h04^m52.6^s	−24°26′35″
SE1	18^h04^m21.6^s	−24°28′17″
SE2	18^h04^m24.4^s	−24°28′39″
SE3	18^h04^m31.1^s	−24°28′53″
SE4	18^h04^m32.9^s	−24°29′08″
SE5	18^h04^m34.4^s	−24°29′05″
SE6	18^h04^m43.1^s	−24°28′32″
SE7	18^h04^m48.5^s	−24°27′33″
SE8^*	18^h04^m50.5^s	−24°26′59″
SC1	18^h03^m47.5^s	−24°25′ 31″
SC2	18^h03^m48.1^s	−24°26′18″
SC3	18^h03^m47.3^s	−24°26′33″
SC4	18^h03^m43.9^s	−24°27′28″
SC5^*	18^h03^m40.7^s	−24°27′59″
SC6	18^h03^m57.6^s	−24°26′22″
SC7	18^h03^m57.0^s	−24°28′12″
SC8	18^h04^m09.5^s	−24°27′30″
SC9	18^h04^m12.2^s	−24°28′58″
C1	18^h03^m54.1^s	−24°25′40″
C2	18^h03^m51.2^s	−24°24′14″
C3	18^h04^m08.2^s	−24°24′30″

Notes. For clumps marked with an asterisk, we used corrected coordinates when observing with the IRAM 30m telescope and when extracting flux density from the dust continuum maps (WC3: 18^h03^m44.8^s, -24°21′03″; SE8: 18^h04^m50.5^s, -24°27′33″; SC5: 18^h03^m40.7^s, −24°26′59″).

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