Open Access

Table A.2.

Definitions and formulae for various observed and calculated parameters in this work.

Term Definition
α, δ Right ascension and declination
l, b Galactic coordinates
ϖ Parallax
α0, δ0 Cluster centre in equatorial coordinates
l0, b0 Cluster centre in Galactic coordinates
Δα Tangential projection of α
=cos(δ)sin(α − α0)
Δδ Tangential projection of δ
=sin(δ)cos(δ0)−cos(δ)sin(δ0)cos(α − α0)
Δl Tangential projection of l
=cos(b)sin(l − l0)
Δb Tangential projection of b
=sin(b)cos(b0)−cos(b)sin(b0)cos(l − l0)
R Projected angular radius from the cluster centre
= Δ l 2 + Δ b 2 $ =\sqrt{\Delta l^2+\Delta b^2} $
ϕ Azimuth in the 2D tangential plane
=tan−1δα)
PA Position angle of spin axis as measured plane
clockwise from Galactic East, in the sky
XR Projected angular distance from the spin axis
= − Δlsin(PA)+Δbcos(PA)
ΔV The difference between the mean RVs of two
cluster sections divided by the assumed spin axis
μα* PM in the right ascension direction
=μα cos δ
μδ PM in the declination direction
RV Radial velocity
μα * ,corr Projection corrected μα* (See Sect. 2.3)
μδ, corr Projection corrected μδ (See Sect. 2.3)
RVcorr Projection corrected RV (See Sect. 2.3)
μR Radial component of the PM
=μα * ,corrcos(−ϕ)−μδ, corrsin(−ϕ)
μT Tangential component of the PM
=μα * ,corrsin(−ϕ)+μδ, corrcos(−ϕ)

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