The jet paths of radio active galactic nuclei and their cluster weather

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Volume 695 (March 2025)

A&A, 695 (2025) A178

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Table 7.

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

BA	N	Median $_{16 %}^{84 %}$ $^{84\%}_{16\%}$
(deg)		BA/deg	z	log₁₀(M₂₀₀/M_⊙)	r/r₂₀₀	kT/keV
> 160	6	$173 . 0_{169.6}^{175.4}$ $173.0^{175.4}_{169.6}$	$0 . 39_{0.26}^{0.61}$ $0.39^{0.61}_{0.26}$	$13 . 96_{13.86}^{14.06}$ $13.96^{14.06}_{13.86}$	$0 . 30_{0.21}^{0.35}$ $0.30^{0.35}_{0.21}$	$1 . 63_{1.53}^{1.85}$ $1.63^{1.85}_{1.53}$
≤160	11	$122 . 0_{70.4}^{141.6}$ $122.0^{141.6}_{70.4}$	$0 . 35_{0.22}^{0.65}$ $0.35^{0.65}_{0.22}$	$13 . 99_{13.76}^{14.25}$ $13.99^{14.25}_{13.76}$	$0 . 15_{0.06}^{0.43}$ $0.15^{0.43}_{0.06}$	$1 . 66_{1.14}^{2.75}$ $1.66^{2.75}_{1.14}$

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 N_gal is the number of radio sources.

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