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Table A.1

Additional parameters of the MDCs.

Data set from Tigé et al. (2017) ALMA-cycle 3 observations


Sourcea RA Dec M/L Ta σcont Mass sensitivity
(J2000) (J2000) (L) (ML−1) (cm−3) (K) (mJy beam−1) (μJy beam−1) at 5σc
NGC 6334-MDC#11 17:20:02.16 −36:12:14.5 110 1.55 2.4 × 105 14.1 15.8 273 0.11 M
NGC 6334-MDC#16 17:19:05.24 −36:07:57.8 11 13.64 1.6 × 106 9.9 15.8 263 0.19 M
NGC 6334-MDC#17 17:19:51.86 −35:57:07.7 230 0.65 4.8 × 106 16.5 16.8 310 0.10 M
NGC 6334-MDC#21 17:20:30.91 −36:00:54.8 390 0.33 2.2 × 105 18.3 16.9 283 0.06 M
NGC 6334-MDC#27 17:19:39.66 −35:56:52.0 120 0.88 1.3 × 106 15.6 16.4 292 0.07 M
NGC 6334-MDC#26 17:20:55.36 −35:46:05.7 740 0.14 7.5 × 106 21.1 17.6 656 0.16 M
NGC 6334-MDC#35 17:19:58.00 −36:13:13.5 140 0.64 3.4 × 105 16.4 17.2 318 0.11 M
NGC 6334-MDC#44 17:22:25.58 −35:16:59.9 27 2.85 1.0 × 105 12.8 16.5 281 0.08 M
NGC 6334-MDC#45 17:17:47.95 −36:09:28.5 60 1.27 2.0 × 106 14.7 16.5 352 0.14 M

Mean 203 2.44 2.0 × 106 15.5 16.6 336 0.11 M

Notes. (a) The source’s name, radius, bolometric luminosity, and density follow the work by Tigé et al. (2017). (b) The 1σ rms noise level is given per channel, where the channel width is 0.7 km s−1. (c) The method to estimate the mass from the 5σ value follows Eq. (2).

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