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Table 5

Bright state XMM-Newton EPIC pn spectral best fit parameters and derived parameters for M31N 2007-12b.

ObsID tint Ratea Spectrab NHc kT ν χ2/ν Lxd Lbole Lbol/L Rf
(ks) (10-3 ct s-1) (1021 cm-2) (eV) (1038 erg s-1) (104) (109 cm)

0505720301 22.08 260  ±  3 BB 78 1.12 7.7 11.0 28.8 2.78
WD H 78 1.36 1.9 2.3 5.9 1.12
WD S 78 1.28 1.6 1.8 4.8 0.78
0505720401 17.94 395 ± 5 BB 96 1.63 6.1 8.4 21.9 1.31
WD H 96 1.47 2.4 2.7 7.2 0.94
WD S 96 1.29 2.6 3.0 7.7 0.85
0505720501 16.86 479 ± 5 BB 112 2.68 7.6 10.2 26.6 1.27
WD H 112 1.06 2.4 2.7 7.0 0.80
WD S 112 0.98 2.4 2.7 6.9 0.71
0505720601 17.42 291 ± 4 BB 71 1.76 3.7 5.0 13.1 1.06
WD H 71 0.93 1.6 1.8 4.7 0.75
WD S 71 0.89 1.6 1.7 4.6 0.61

Notes. 

(a)

Net count rate as given in XSPEC (0.15–1 keV);

(b)

model spectra. BB: black-body, WD H and WD S: NLTE WD atmosphere assuming Galactic halo or solar abundances, respectively (see text);

(c)

absorption with Galactic metal abundances (Wilms et al. 2000);

(d)

un-absorbed X-ray luminosity (0.15–1 keV);

(e)

bolometric luminosity;

(f)

WD radii, for WD atmosphere models calculated as for BB.

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