A three-dimensional reconstruction of the interstellar magnetic field toward a star-forming region

Open Access

Table 2

List of the seven clouds, ℂ_i (i = 1, …, 7), identified toward the G139 region.

Cloud Kinematic components	${\bar{p}}_{d, i}$ ${{\bar p}_{{\rm{d}},i}}$	${\bar{ψ}}_{d, i}$ ${{\bar \psi }_{{\rm{d}},i}}$
ℂ₁ Hi [1]	22.9 ±0.1	5.2 ± 1.3
ℂ₂ Hi [2-3]	6.4 ± 0.2	16.8 ±0.8
ℂ₃ Hi [4]	14.2 ±0.4	89.4 ±0.9
ℂ₄ Hi [5-6], CO [3-4]	2.2 ± 0.2	46.3 ± 1.9
ℂ₅ Hi [7-19], CO [5-6]	17.9 ± 0.1	-3.4 ± 0.2
ℂ₆ CO [1-2]	5.8 ± 0.3	66.1 ± 1.7
ℂ₇ CO [7]	22.5 ± 0.5	-21.2 ±3.4

Notes. ^(a) Best-fit value and standard deviation of the polarization fraction of cloud ℂ_i. ^(b) Best-fit value and standard deviation of the polarization angle of cloud ℂ_i. The boxed values pertain to the two most interesting molecular clouds: the bright CO core, ℂ₆ (bold style), and the oblique, elongated cloud, ℂ₄ (normal style).

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