ALMA resolves molecular clouds in metal-poor Magellanic Bridge A

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Table 6

Characteristics of the clouds identified in the CO(2−1) line cube.

CO Source	RA	Dec	A	Peak	v_LSR ^(b)	Δv (FWHM) ^(b)	S_CO(2−1)Δv ^(b)
	(J2000)	(J2000)	(pc²)	(Jy beam⁻¹ km s⁻¹)	(km s⁻¹)	(km s⁻¹)	(Jy km s⁻¹)
North	1:43:49.2	−74:32:00.6	8.1	1.67 ± 0.05	174.6 ± 0.6	1.33 ± 0.03	30.67 ± 2.86
South	1:43:53.8	−74:32:24.7	5.8	2.81 ± 0.05	174.0 ± 0.9	1.93 ± 0.05	21.65 ± 2.05

Notes. ^(a) Peak values obtained from the CO(2−1) integrated line image between 172 and 176 km s⁻¹. ^(b) Values obtained from the Gaussian fit to the integrated spectra over the cloud area.

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