Open Access

Table 5

Main parameters of the 11 areas with associated massive star candidates.

Area n Dist Gaia¯dcMathematical equation: $\[\overline{Gaia}_{d c}\]$ E(BV)¯cMathematical equation: $\[\overline{E_{(B-V)}} c\]$ E(BV) E(B–V)m E(B–V)M
(kpc) (mag)
A1 5 2.4±0.3 2.1 0.5 0.7 0.4 1.0
A2 2 2.4 2.4±0.1 1.6 1.5 1.4 1.9
A3 13 2.8±0.1 2.8±0.1 0.8 0.7 0.5 1.0
A4 35 2.6±0.3 2.8±0.1 1.7 1.7 1.6 1.8
A5 1 2.8 0.7 0.5 1.0
A6 1 3.0 0.7 0.5 1.0
A7 2 2.4±0.1 0.7 0.5 1.0
A8 5 2.8±0.1 0.7 0.5 1.0
A9 18 2.7±0.3 0.7 0.5 1.0
A10 23 3.0±0.2 0.7 0.5 1.0
A11 1 2.8 0.7 0.5 1.0

Notes. For each of 11 areas with associated massive star candidates, table lists number of massive star candidates (n), weighted average distance and its weighted standard deviation (Dist.) computed from n individual values given by Bailer-Jones et al. (2021), weighted average distance and its weighted standard deviation, and average colour excess derived from confirmed OB-type stars listed in Table 4. Additionally, we provide the colour excess and its adopted range.

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.