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Table 6.

Median X-ray group properties and percentiles for straight (BA >  160 deg) and bent (BA ≤ 160 deg) group members in the COSMOS sample.

BA N Median 16 % 84 % $ ^{84\%}_{16\%} $
(deg) BA/deg z log10(M200/M) r/r200 kT/keV Ngal
> 160 7 171 . 0 164.9 174.1 $ 171.0^{174.1}_{164.9} $ 0 . 44 0.36 0.90 $ 0.44^{0.90}_{0.36} $ 13 . 81 13.59 13.87 $ 13.81^{13.87}_{13.59} $ 0 . 19 0.06 0.52 $ 0.19^{0.52}_{0.06} $ 1 . 28 0.99 1.69 $ 1.28^{1.69}_{0.99} $ 20 . 0 11 83 $ 20.0^{83}_{11} $
≤160 12 134 . 5 89.2 156.5 $ 134.5^{156.5}_{89.2} $ 0 . 34 0.21 0.41 $ 0.34^{0.41}_{0.21} $ 13 . 56 13.29 13.97 $ 13.56^{13.97}_{13.29} $ 0 . 14 0.03 0.41 $ 0.14^{0.41}_{0.03} $ 0 . 88 0.64 1.74 $ 0.88^{1.74}_{0.64} $ 22 . 5 7 117 $ 22.5^{117}_{7} $

Notes. BA is the bending angle in degrees; z the redshift; M200 is the mass of the galaxy group in M; r is the distance from the X-ray galaxy group centre normalised to r200; kT is the temperature of the group in kilo-electronvolts; and Ngal is the number of galaxies that are members of the X-ray galaxy group.

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