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Table 2

Spectral parameters of known members.

RECX  NH k T1 k T2 k T3 EM1/EM2 EM1/EM3 Z χ2 (d.o.f.) Unabsorbed fX log LX log LX**
(× 1021 cm-2) (keV) (keV) (keV) (Z) (× 10-13 erg cm-2 s-1) (erg s-1) (erg s-1)

3 0.00 0.63 ... ... ... ... 0.08 1.12 (88) 0.65 28.9 29.2
4 0.44 0.28 0.96 ... 0.92 ... 0.12 1.29 (402) 6.61 29.9 30.2
5 0.00 0.27 0.74 ... 1.30 ... 0.10 0.96 (162) 0.56 28.8 29.1
6 0.23 0.33 0.95 ... 0.88 ... 0.13 0.93 (347) 2.47 29.4 29.6
7 0.03 0.33 0.94 2.08 0.75 2.21 0.19 1.03 (491) 10.50 30.1 30.4
8 0.00 0.26 0.76 1.54 0.87 0.61 0.26 1.28 (353) 4.05 29.7 29.9
9 2.89 0.77 2.22 ... 0.47 ... 0.30 1.12 (518) 2.95 29.5 28.5
10 0.04 0.40 0.98 ... 0.72 ... 0.15 0.92 (300) 4.07 29.7 30.0
11 0.06 0.25 0.95 2.52 0.90 1.20 0.21 1.20 (805) 27.93 30.5 30.2
12 0.11 0.28 1.00 2.90 0.73 2.45 0.20 ... 10.90 30.1 30.2
14* ... ... ... ... ... ... ... ... ... ... ...
15 1.27 0.80 ... ... ... ... 0.04 1.05 (64) 0.31 28.8 ...

Notes.

(*)

The background subtracted spectrum of RECX 14 has only 67 counts. We failed any attempt of fitting a plasma model.

(**)

X-ray luminosities determined by Mamajek et al. (2000) in the 0.1−2.0 ROSAT energy band.

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