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Table 1.

Investigated objects and extracted proper motions, including clusters and YSOs with published astrometric data.

Object α δ μα* μδ Source
[°] [°] [mas yr−1] [mas yr−1]
CrA ISM VISIONS 1 285.480917 –36.951804 17.5 ± 0.7 –34.5 ± 0.8 VISIONS, this work
CrA ISM VISIONS 2 285.483364 –36.955935 16.8 ± 2.3 –21.5 ± 1.3 VISIONS, this work
CrA ISM VISIONS 3 285.492770 –36.957004 2.8 ± 5.3 –30.6 ± 4.7 VISIONS, this work

HH 99B 285.524000 –36.910536 48.9 ± 4.4 1.9 ± 4.6 VISIONS, this work
CrA ISM VISIONS HH 285.552603 –36.945413 73.2 ± 10.5 –2.1 ± 17.2 VISIONS, this work
CHLT 15 285.494067 –36.952587 –2.6 ± 3.3 –28.4 ± 5.1 VISIONS, this work

R CrA 285.4737 –36.9524 7.6 ± 0.5 –20.9 ± 0.5 Gaia DR3
CrA-North 280.1330 –36.3063 0.7 ± 2.1 –27.6 ± 1.2 Gaia DR3, Ratzenböck et al. (2023a)
CrA-Main 285.0759 –36.9739 4.8 ± 1.0 –27.2 ± 1.2 Gaia DR3, Ratzenböck et al. (2023a)
CrA YSOs 285.1298 –37.1894 5.0 ± 1.0 –27.4 ± 1.0 Gaia DR3, this work (Appendix C)

Notes. Assuming a distance of 150 pc (Posch et al. 2023, and references therein), velocities in km s−1 can be roughly estimated as vi = 0.711 μi.

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