Open Access

Table F.2.

Astrometric parameters of the questionable runaway candidates.

Star α [h m s] δ [d m s] π [mas] μ α Mathematical equation: $ \mu_{\alpha}^{*} $ [mas/yr] μδ [mas/yr] vrad [km/s] Ref. vrad
Cl* NGC 2264 VAS 133 06 41 09.9986 +09 27 46.0740 1.76±0.20 -2.48±0.20 -2.54±0.16 120.60±2.00 (4)
Gaia DR3 4096398244806369792 18 17 23.6627 -18 14 14.8172 0.71±0.11 1.00±0.13 -0.71±0.10 221.33±26.69 (1)
Gaia DR3 4111239113458529152 17 26 57.8761 -24 15 12.7072 0.61±0.04 2.24±0.05 -1.61±0.03 635.55±8.26 (1)

Notes. For all three stars, coordinates α and δ, parallaxes π as well as proper motions μ α Mathematical equation: $ \mu_{\alpha}^{*} $ and μδ were taken from Gaia DR3. References for the presented radial velocities vrad are indicated by the following indices: (1): Gaia DR3; (4): Jönsson et al. (2020).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.