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This article has an erratum: [https://doi.org/10.1051/0004-6361/202142281e]


Table A.1.

Summary of sightlines used to determine distance limits to clouds.

Cloud l (°) b (°) dnew (pc) dold (pc) Ref.
IC 5146 93.7 -4.6 774 460 (1)
IC 5146 93.4 -4.2 792 460 (1)
IC 5146 94.0 -4.9 730 460 (1)
IC 5146 94.4 -5.5 751 460 (1)
Orion B 205.7 -14.8 436 460 (1)
Orion B 207.9 -16.8 411 460 (1)
Orion B 207.4 -16.0 451 460 (1)
Orion B 204.8 -13.3 415 460 (1)
Taurus 171.6 -15.8 130 140 (1)
Ophiuchus 352.7 15.4 139 140 (1)
Ophiuchus 353.2 16.6 139 140 (1)
Aquila 28.4 3.9 250±5 260 (2)
Aquila 28.8 4.1 250±5 260 (2)
Aquila 28.6 3.2 250±5 260 (2)
Aquila 28.6 3.8 250±5 260 (2)
Aquila 28.7 3.5 250±5 260 (2)
Aquila 26.8 3.4 260±5 260 (2)
Polaris 124.3 25.3 355±5 150 (2)
Polaris 123.7 24.8 355±5 150 (2)
Polaris 123.7 25.2 355±5 150 (2)
Polaris 123.3 24.9 350±5 150 (2)
Polaris 124.7 25.2 360±5 150 (2)
Musca 301.2 -8.4 170±5 200 (2)
Musca 300.8 -9.1 170±5 200 (2)
Pipe 0.0 4.6 155±5 145 (2)
Pipe 358.6 5.9 150±5 145 (2)
Pipe 357.2 6.9 150±5 145 (2)
Pipe 357.7 6.6 150±5 145 (2)

Notes. Columns are cloud name, galactic coordinates of each sightline, new distance, distance originally adopted by Arzoumanian et al. (2019), and reference for the new distance – (1) for Zucker et al. (2020), (2) for this work.

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