ALMA resolves molecular clouds in metal-poor Magellanic Bridge A

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Table 4

Gas masses and best fit MBB parameters to the cloud SEDs.

Source	C (sr Hz^−β)	β	T_d (K)	χ²	M_gas (10³ M_⊙) ^(‡)
MagBridgeA ^(*)	(1.9 ± 23.4) × 10⁻²⁹	1.4 ± 0.5	22.4 ± 3.4	0.27	6.8 ± 1.5
North^(**)	(9.0 ± 3.1) × 10⁻³⁰	1.4^(†)	21.7 ± 2.2	0.5	1.3 ± 0.5
South^(**)	(2.1 ± 0.4) × 10⁻²⁹	1.4^(†)	24.5 ± 1.1	0.04	2.9 ± 0.5

Notes. ^(*) Fluxes measured using aperture photometry radius of 50′′. ^(**) Fluxes measured using aperture photometry radius of 11′′. ^(†) β values obtained for Magellanic Bridge A MBB fit. ^(‡)Gas masses derived from the MBB models that best fit the FIR SEDs of each source.

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