The long X-ray tail in Zwicky 8338

G. Schellenberger; T. H. Reiprich

doi:10.1051/0004-6361/201527317

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Volume 583 (November 2015)

A&A, 583 (2015) L2

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Table 2

Best-fit temperature, relative abundance of heavy elements, X-ray luminosity, and signal-to-noise ratio using a redshift of 0.0501.

Region	kT	Z	L_0.5−2	S/N
	keV	Z_⊙	10⁴³ erg s^-1

Head
Tail
Full Comet

Head^*				10
Main tail^*				11
Full comet^*				14

Outside^*		0.05 fixed		5

Notes. The

^(*)

marks fits, where the cluster emission in (4–7)′ was simultaneously fitted and accounted for (the S/N could only in these cases be calculated properly, since the cluster emission is accounted for in the noise).

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